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Cinema MK2, 14 quai de la Seine Paris 19th arrondissement.
Cinema MK2, 14 quai de la Seine Paris 19th arrondissement.

TEC4613814: Cinema MK2, 14 quai de la Seine Paris 19th arrondissement. / Bridgeman Images

ID: TEC4613814

Cinema MK2, 14 quai de la Seine Paris 19th arrondissement.

Internal view of the church of Porto Rotondo (photography)
Internal view of the church of Porto Rotondo (photography)

LRI4614001: Internal view of the church of Porto Rotondo (photography), Ceroli, Mario (b.1938) / Bridgeman Images

ID: LRI4614001

Internal view of the church of Porto Rotondo (photography)

Ceroli, Mario (b.1938)

Le Rialto, Grand hotel of Flanders, rue de Flanders in Paris 19th.
Le Rialto, Grand hotel of Flanders, rue de Flanders in Paris 19th.

MDA4614410: Le Rialto, Grand hotel of Flanders, rue de Flanders in Paris 19th. / Bridgeman Images

ID: MDA4614410

Le Rialto, Grand hotel of Flanders, rue de Flanders in Paris 19th.

Bassin de la Villette in Paris 19th. Photography 1988.
Bassin de la Villette in Paris 19th. Photography 1988.

MDA4614457: Bassin de la Villette in Paris 19th. Photography 1988. / Bridgeman Images

ID: MDA4614457

Bassin de la Villette in Paris 19th. Photography 1988.

Carrefour du vieux Paris, boulevard de la Chapelle et de la rue de Flandre, Paris 19th. Photography 1988.
Carrefour du vieux Paris, boulevard de la Chapelle et de la rue de Flandre, Paris 19th. Photography 1988.

MDA4614523: Carrefour du vieux Paris, boulevard de la Chapelle et de la rue de Flandre, Paris 19th. Photography 1988. / Bridgeman Images

ID: MDA4614523

Carrefour du vieux Paris, boulevard de la Chapelle et de la rue de Flandre, Paris 19th. Photography 1988.

Rotunda by Claude Nicolas Ledoux (1736-1806) Place Stalingrad, Paris 75019. It is one of the four remains of the enclosure of the Farmers Generaux with that of the Monceau parks, Denfert Rochereau and the columns of the Trone. Built in 1786, this rotunda evokes the Rotonda de Palladio in Vicenze (Italy). This barrier served as a gendarmerie barracks from 1830 to 1860, and then as a storage room for salt. Restauree under the direction of Bernard Huet, it is now occupied by the Commission du Vieux Paris.
Rotunda by Claude Nicolas Ledoux (1736-1806) Place Stalingrad, Paris 75019. It is one of the four remains of the enclosure of the Farmers Generaux with that of the Monceau parks, Denfert Rochereau and the columns of the Trone. Built in 1786, this rotunda evokes the Rotonda de Palladio in Vicenze (Italy). This barrier served as a gendarmerie barracks from 1830 to 1860, and then as a storage room for salt. Restauree under the direction of Bernard Huet, it is now occupied by the Commission du Vieux Paris.

MDA4614573: Rotunda by Claude Nicolas Ledoux (1736-1806) Place Stalingrad, Paris 75019. It is one of the four remains of the enclosure of the Farmers Generaux with that of the Monceau parks, Denfert Rochereau and the columns of the Trone. Built in 1786, this rotunda evokes the Rotonda de Palladio in Vicenze (Italy). This barrier served as a gendarmerie barracks from 1830 to 1860, and then as a storage room for salt. Restauree under the direction of Bernard Huet, it is now occupied by the Commission du Vieux Paris. / Bridgeman Images

ID: MDA4614573

Rotunda by Claude Nicolas Ledoux (1736-1806) Place Stalingrad, Paris 75019. It is one of the four remains of the enclosure of the Farmers Generaux with that of the Monceau parks, Denfert Rochereau and the columns of the Trone. Built in 1786, this rotunda evokes the Rotonda de Palladio in Vicenze (Italy). This barrier served as a gendarmerie barracks from 1830 to 1860, and then as a storage room for salt. Restauree under the direction of Bernard Huet, it is now occupied by the Commission du Vieux Paris.

Earth and Moon - Artist view - Earth and Moon. Artwork - Earth with starry sky - Earth's equatorial diameter is 12.756 km while the Moon's diameter is 3.476 km
Earth and Moon - Artist view - Earth and Moon. Artwork - Earth with starry sky - Earth's equatorial diameter is 12.756 km while the Moon's diameter is 3.476 km

PIX4614588: Earth and Moon - Artist view - Earth and Moon. Artwork - Earth with starry sky - Earth's equatorial diameter is 12.756 km while the Moon's diameter is 3.476 km / Bridgeman Images

ID: PIX4614588

Earth and Moon - Artist view - Earth and Moon. Artwork - Earth with starry sky - Earth's equatorial diameter is 12.756 km while the Moon's diameter is 3.476 km

Full Moon - Sardinia - Full Moon - Sardinia
Full Moon - Sardinia - Full Moon - Sardinia

PIX4614625: Full Moon - Sardinia - Full Moon - Sardinia / Bridgeman Images

ID: PIX4614625

Full Moon - Sardinia - Full Moon - Sardinia

The Rotonde flood in Paris 19th century.
The Rotonde flood in Paris 19th century.

MDA4614682: The Rotonde flood in Paris 19th century. / Bridgeman Images

ID: MDA4614682

The Rotonde flood in Paris 19th century.

Proun Watercolour by Lazar Lissitskij dit El Lissitskij (Lissitsky or Lissitzky or Lissitzky) (1890-1941) 1924 Stedelijk Van Abbemuseum Eindhoven
Proun Watercolour by Lazar Lissitskij dit El Lissitskij (Lissitsky or Lissitzky or Lissitzky) (1890-1941) 1924 Stedelijk Van Abbemuseum Eindhoven

LRI4614731: Proun Watercolour by Lazar Lissitskij dit El Lissitskij (Lissitsky or Lissitzky or Lissitzky) (1890-1941) 1924 Stedelijk Van Abbemuseum Eindhoven, Lissitzky, (El) Eliezer Markowich (1890-1941) / Bridgeman Images

ID: LRI4614731

Proun Watercolour by Lazar Lissitskij dit El Lissitskij (Lissitsky or Lissitzky or Lissitzky) (1890-1941) 1924 Stedelijk Van Abbemuseum Eindhoven

Lissitzky, (El) Eliezer Markowich (1890-1941)

Eclipse de Lune - 28/09/2015 - Lunar eclipse September 28 2015: Total Eclipse of Moon of 28 September 2015
Eclipse de Lune - 28/09/2015 - Lunar eclipse September 28 2015: Total Eclipse of Moon of 28 September 2015

PIX4614775: Eclipse de Lune - 28/09/2015 - Lunar eclipse September 28 2015: Total Eclipse of Moon of 28 September 2015 / Bridgeman Images

ID: PIX4614775

Eclipse de Lune - 28/09/2015 - Lunar eclipse September 28 2015: Total Eclipse of Moon of 28 September 2015

Wall painting in Paris 10th. Photography 10/06/99.
Wall painting in Paris 10th. Photography 10/06/99.

TEC4614933: Wall painting in Paris 10th. Photography 10/06/99. / Bridgeman Images

ID: TEC4614933

Wall painting in Paris 10th. Photography 10/06/99.

Statue of Jean-Dominique Cassini in Paris - Giovanni Dominico Cassini Statue -Paris: View of the statue of Giovanni Dominico Cassini (1625-1712), in the courtyard Napoleon of the Louvre. At the request of Louis XIV, he became the first director of the Paris Observatory from 1671
Statue of Jean-Dominique Cassini in Paris - Giovanni Dominico Cassini Statue -Paris: View of the statue of Giovanni Dominico Cassini (1625-1712), in the courtyard Napoleon of the Louvre. At the request of Louis XIV, he became the first director of the Paris Observatory from 1671

PIX4614019: Statue of Jean-Dominique Cassini in Paris - Giovanni Dominico Cassini Statue -Paris: View of the statue of Giovanni Dominico Cassini (1625-1712), in the courtyard Napoleon of the Louvre. At the request of Louis XIV, he became the first director of the Paris Observatory from 1671 / Bridgeman Images

ID: PIX4614019

Statue of Jean-Dominique Cassini in Paris - Giovanni Dominico Cassini Statue -Paris: View of the statue of Giovanni Dominico Cassini (1625-1712), in the courtyard Napoleon of the Louvre. At the request of Louis XIV, he became the first director of the Paris Observatory from 1671

Nebula of the Horse's Head (IC 434) in Orion - Nebula of the Horse's Head (IC 434) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the nebula has emitting IC 434 about 1500 years - light of the Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergeant star belonging to the Orion Baudrier. Towards the center of the image, a reflexion nebula, NGC 2023
Nebula of the Horse's Head (IC 434) in Orion - Nebula of the Horse's Head (IC 434) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the nebula has emitting IC 434 about 1500 years - light of the Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergeant star belonging to the Orion Baudrier. Towards the center of the image, a reflexion nebula, NGC 2023

PIX4622002: Nebula of the Horse's Head (IC 434) in Orion - Nebula of the Horse's Head (IC 434) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the nebula has emitting IC 434 about 1500 years - light of the Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergeant star belonging to the Orion Baudrier. Towards the center of the image, a reflexion nebula, NGC 2023 / Bridgeman Images

ID: PIX4622002

Nebula of the Horse's Head (IC 434) in Orion - Nebula of the Horse's Head (IC 434) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the nebula has emitting IC 434 about 1500 years - light of the Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergeant star belonging to the Orion Baudrier. Towards the center of the image, a reflexion nebula, NGC 2023

Nebula of the horse's head in Orion (IC 434) - The Horsehead is located in the constellation of Orion, slightly below the left - most star of the three that form the Hunter's belt. It is part of a vast molecular cloud of dust and gas that includes the Great Orion Nebula and extends throughout the entire constellation as well. It was first seen through photographs taken by E. Pickering in January 1900. The red coloration is the result of glowing hydrogen gas located primarily behind the formation. Here, we see the Horsehead as it appeared 1,500 years ago, due to distance and the time it takes light to travel. The bright complex of dust and gas below the Horsehead reflects the light given off by the bright star near it's center and is one of the brightest examples of reflection nebulae in the northern sky. The central star is surrounded with a thin shell of hydrogen that glows red by emitting it's own light in a rare example of a unique process called vibrational fluorescence. There are also an number of dark clumps of gas that represent stellar nurseries containing one or more new stars hidden within. The Horsehead can be challenging to see visually, but under very dark skies, many observers report that it can be glimpsed in silhouette with a ten inch telescope and an H - beta filter that accentuates the background hydrogen glow
Nebula of the horse's head in Orion (IC 434) - The Horsehead is located in the constellation of Orion, slightly below the left - most star of the three that form the Hunter's belt. It is part of a vast molecular cloud of dust and gas that includes the Great Orion Nebula and extends throughout the entire constellation as well. It was first seen through photographs taken by E. Pickering in January 1900. The red coloration is the result of glowing hydrogen gas located primarily behind the formation. Here, we see the Horsehead as it appeared 1,500 years ago, due to distance and the time it takes light to travel. The bright complex of dust and gas below the Horsehead reflects the light given off by the bright star near it's center and is one of the brightest examples of reflection nebulae in the northern sky. The central star is surrounded with a thin shell of hydrogen that glows red by emitting it's own light in a rare example of a unique process called vibrational fluorescence. There are also an number of dark clumps of gas that represent stellar nurseries containing one or more new stars hidden within. The Horsehead can be challenging to see visually, but under very dark skies, many observers report that it can be glimpsed in silhouette with a ten inch telescope and an H - beta filter that accentuates the background hydrogen glow

PIX4622024: Nebula of the horse's head in Orion (IC 434) - The Horsehead is located in the constellation of Orion, slightly below the left - most star of the three that form the Hunter's belt. It is part of a vast molecular cloud of dust and gas that includes the Great Orion Nebula and extends throughout the entire constellation as well. It was first seen through photographs taken by E. Pickering in January 1900. The red coloration is the result of glowing hydrogen gas located primarily behind the formation. Here, we see the Horsehead as it appeared 1,500 years ago, due to distance and the time it takes light to travel. The bright complex of dust and gas below the Horsehead reflects the light given off by the bright star near it's center and is one of the brightest examples of reflection nebulae in the northern sky. The central star is surrounded with a thin shell of hydrogen that glows red by emitting it's own light in a rare example of a unique process called vibrational fluorescence. There are also an number of dark clumps of gas that represent stellar nurseries containing one or more new stars hidden within. The Horsehead can be challenging to see visually, but under very dark skies, many observers report that it can be glimpsed in silhouette with a ten inch telescope and an H - beta filter that accentuates the background hydrogen glow / Bridgeman Images

ID: PIX4622024

Nebula of the horse's head in Orion (IC 434) - The Horsehead is located in the constellation of Orion, slightly below the left - most star of the three that form the Hunter's belt. It is part of a vast molecular cloud of dust and gas that includes the Great Orion Nebula and extends throughout the entire constellation as well. It was first seen through photographs taken by E. Pickering in January 1900. The red coloration is the result of glowing hydrogen gas located primarily behind the formation. Here, we see the Horsehead as it appeared 1,500 years ago, due to distance and the time it takes light to travel. The bright complex of dust and gas below the Horsehead reflects the light given off by the bright star near it's center and is one of the brightest examples of reflection nebulae in the northern sky. The central star is surrounded with a thin shell of hydrogen that glows red by emitting it's own light in a rare example of a unique process called vibrational fluorescence. There are

Horsehead Nebula (IC 434) in Orion - Horsehead Nebula (B33) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - light from Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergiant star belonging to the Baudrier of Orion. Towards the center of the image, a reflexion nebula, NGC 2023. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. This distinctive red emission nebula (IC 434) is the result of radiation from sigma Orionis interacting with the surface of a dusty cloud of gas from which projects the dark shape of the head of a horse. Sigma is the second brightest star in the picture and is at about the same distance from the Sun as the nebula. The brightest star here is zeta Orionis, easily visible to the unaided eye as the easternmost star in the line of three which form Orion's Belt. Alnitak (Zeta Orionis) is a supergiant star with a brightness 35,000 times greater than the Sun. Its mass is 20 times the solar mass. Partly obscured by the glare of zeta is the curious yellowish nebula NGC 2024, whose energy comes from stars hidden in the dark lane, while other nebulae simply reflect the light of embedded hot stars and appear blue. All these objects are about 1500 light years distant. This photograph was produced by combining three separate photographs taken with the 1.2m UK Schmidt Telescope through different coloured filters
Horsehead Nebula (IC 434) in Orion - Horsehead Nebula (B33) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - light from Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergiant star belonging to the Baudrier of Orion. Towards the center of the image, a reflexion nebula, NGC 2023. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. This distinctive red emission nebula (IC 434) is the result of radiation from sigma Orionis interacting with the surface of a dusty cloud of gas from which projects the dark shape of the head of a horse. Sigma is the second brightest star in the picture and is at about the same distance from the Sun as the nebula. The brightest star here is zeta Orionis, easily visible to the unaided eye as the easternmost star in the line of three which form Orion's Belt. Alnitak (Zeta Orionis) is a supergiant star with a brightness 35,000 times greater than the Sun. Its mass is 20 times the solar mass. Partly obscured by the glare of zeta is the curious yellowish nebula NGC 2024, whose energy comes from stars hidden in the dark lane, while other nebulae simply reflect the light of embedded hot stars and appear blue. All these objects are about 1500 light years distant. This photograph was produced by combining three separate photographs taken with the 1.2m UK Schmidt Telescope through different coloured filters

PIX4622070: Horsehead Nebula (IC 434) in Orion - Horsehead Nebula (B33) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - light from Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergiant star belonging to the Baudrier of Orion. Towards the center of the image, a reflexion nebula, NGC 2023. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. This distinctive red emission nebula (IC 434) is the result of radiation from sigma Orionis interacting with the surface of a dusty cloud of gas from which projects the dark shape of the head of a horse. Sigma is the second brightest star in the picture and is at about the same distance from the Sun as the nebula. The brightest star here is zeta Orionis, easily visible to the unaided eye as the easternmost star in the line of three which form Orion's Belt. Alnitak (Zeta Orionis) is a supergiant star with a brightness 35,000 times greater than the Sun. Its mass is 20 times the solar mass. Partly obscured by the glare of zeta is the curious yellowish nebula NGC 2024, whose energy comes from stars hidden in the dark lane, while other nebulae simply reflect the light of embedded hot stars and appear blue. All these objects are about 1500 light years distant. This photograph was produced by combining three separate photographs taken with the 1.2m UK Schmidt Telescope through different coloured filters / Bridgeman Images

ID: PIX4622070

Horsehead Nebula (IC 434) in Orion - Horsehead Nebula (B33) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - light from Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergiant star belonging to the Baudrier of Orion. Towards the center of the image, a reflexion nebula, NGC 2023. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. This distinctive red emission nebula (IC 434) is the result of radiation from sigma Orionis interacting with the surface of a dusty cloud of gas from which projects the dark shape of the head of a horse. Sigma is the second brightest star in the picture and is at about the same distance from the Sun as the nebula. The brightest star here is zeta Orionis, easily visible to the unaided eye as the easternmost star in the line of three which form Orion's Belt. Alnitak (Zeta Orionis) is a supergiant sta

Nebula VDB 141 in Cephee - Ghost nebula in Cepheus - VDB 141, is a nebula by reflexion illuminated by the young star BD+67 1300. The reflection nebula VDB 141, the Ghost nebula, is illuminated by a young FU Ori star, BD+67 1300
Nebula VDB 141 in Cephee - Ghost nebula in Cepheus - VDB 141, is a nebula by reflexion illuminated by the young star BD+67 1300. The reflection nebula VDB 141, the Ghost nebula, is illuminated by a young FU Ori star, BD+67 1300

PIX4621536: Nebula VDB 141 in Cephee - Ghost nebula in Cepheus - VDB 141, is a nebula by reflexion illuminated by the young star BD+67 1300. The reflection nebula VDB 141, the Ghost nebula, is illuminated by a young FU Ori star, BD+67 1300 / Bridgeman Images

ID: PIX4621536

Nebula VDB 141 in Cephee - Ghost nebula in Cepheus - VDB 141, is a nebula by reflexion illuminated by the young star BD+67 1300. The reflection nebula VDB 141, the Ghost nebula, is illuminated by a young FU Ori star, BD+67 1300

Dark Nebula in Scorpio - A dark cloud in Scorpius, wide field - This dark nebula is located about 5000 years from Earth. Image obtained by Siding Spring's 3.9m telescope. This curious un - named nebula is governed by radiation from very luminous stars some distance from the nebula. The direction of the radiation source can be seen from the flow pattern in the dark cloud and the extensive bright red rims at the end of the nebula that is exposed to radiation from the hot stars. This part of the nebula is reminiscent of the famous Horsehead nebula in Orion, which is also the consequence of starlight destroying a dark cloud. The source of the energy here is the Scorpius OB association, a group of brilliant, very hot stars, about 5000 light years away from us
Dark Nebula in Scorpio - A dark cloud in Scorpius, wide field - This dark nebula is located about 5000 years from Earth. Image obtained by Siding Spring's 3.9m telescope. This curious un - named nebula is governed by radiation from very luminous stars some distance from the nebula. The direction of the radiation source can be seen from the flow pattern in the dark cloud and the extensive bright red rims at the end of the nebula that is exposed to radiation from the hot stars. This part of the nebula is reminiscent of the famous Horsehead nebula in Orion, which is also the consequence of starlight destroying a dark cloud. The source of the energy here is the Scorpius OB association, a group of brilliant, very hot stars, about 5000 light years away from us

PIX4621577: Dark Nebula in Scorpio - A dark cloud in Scorpius, wide field - This dark nebula is located about 5000 years from Earth. Image obtained by Siding Spring's 3.9m telescope. This curious un - named nebula is governed by radiation from very luminous stars some distance from the nebula. The direction of the radiation source can be seen from the flow pattern in the dark cloud and the extensive bright red rims at the end of the nebula that is exposed to radiation from the hot stars. This part of the nebula is reminiscent of the famous Horsehead nebula in Orion, which is also the consequence of starlight destroying a dark cloud. The source of the energy here is the Scorpius OB association, a group of brilliant, very hot stars, about 5000 light years away from us / Bridgeman Images

ID: PIX4621577

Dark Nebula in Scorpio - A dark cloud in Scorpius, wide field - This dark nebula is located about 5000 years from Earth. Image obtained by Siding Spring's 3.9m telescope. This curious un - named nebula is governed by radiation from very luminous stars some distance from the nebula. The direction of the radiation source can be seen from the flow pattern in the dark cloud and the extensive bright red rims at the end of the nebula that is exposed to radiation from the hot stars. This part of the nebula is reminiscent of the famous Horsehead nebula in Orion, which is also the consequence of starlight destroying a dark cloud. The source of the energy here is the Scorpius OB association, a group of brilliant, very hot stars, about 5000 light years away from us

Saint John a Patmos. Painting by Paolo di Dono dit Paolo Uccello (1397-1475), 1435-1440. Predelle of Quarata. Tempera on wood. Dim: 20x178cm. Florence, Museo Arcivescovile di Cestello.
Saint John a Patmos. Painting by Paolo di Dono dit Paolo Uccello (1397-1475), 1435-1440. Predelle of Quarata. Tempera on wood. Dim: 20x178cm. Florence, Museo Arcivescovile di Cestello.

LRI4621567: Saint John a Patmos. Painting by Paolo di Dono dit Paolo Uccello (1397-1475), 1435-1440. Predelle of Quarata. Tempera on wood. Dim: 20x178cm. Florence, Museo Arcivescovile di Cestello., Uccello, Paolo (1397-1475) / Bridgeman Images

ID: LRI4621567

Saint John a Patmos. Painting by Paolo di Dono dit Paolo Uccello (1397-1475), 1435-1440. Predelle of Quarata. Tempera on wood. Dim: 20x178cm. Florence, Museo Arcivescovile di Cestello.

Uccello, Paolo (1397-1475)

Nebula VDB 10 in Cephee - Nebula VDB 10 in Cepheus - VDB 10 is a nebula by light reflexion. Faint reflection nebula
Nebula VDB 10 in Cephee - Nebula VDB 10 in Cepheus - VDB 10 is a nebula by light reflexion. Faint reflection nebula

PIX4621727: Nebula VDB 10 in Cephee - Nebula VDB 10 in Cepheus - VDB 10 is a nebula by light reflexion. Faint reflection nebula / Bridgeman Images

ID: PIX4621727

Nebula VDB 10 in Cephee - Nebula VDB 10 in Cepheus - VDB 10 is a nebula by light reflexion. Faint reflection nebula

Nebula VDB 123 in Snake - Nebula VDB 123 in Serpens - VDB 123 is a nebula by light reflexion. This region of Serpens contains what is referred to as the Serpens Cloud. It has been cataloged in Herbst, Beckwith, Robberto, 1997 Astrophys. J. This super cloud of dust contains many reflection nebulae, one of which is vdB 123. This is the blue reflection nebula
Nebula VDB 123 in Snake - Nebula VDB 123 in Serpens - VDB 123 is a nebula by light reflexion. This region of Serpens contains what is referred to as the Serpens Cloud. It has been cataloged in Herbst, Beckwith, Robberto, 1997 Astrophys. J. This super cloud of dust contains many reflection nebulae, one of which is vdB 123. This is the blue reflection nebula

PIX4621775: Nebula VDB 123 in Snake - Nebula VDB 123 in Serpens - VDB 123 is a nebula by light reflexion. This region of Serpens contains what is referred to as the Serpens Cloud. It has been cataloged in Herbst, Beckwith, Robberto, 1997 Astrophys. J. This super cloud of dust contains many reflection nebulae, one of which is vdB 123. This is the blue reflection nebula / Bridgeman Images

ID: PIX4621775

Nebula VDB 123 in Snake - Nebula VDB 123 in Serpens - VDB 123 is a nebula by light reflexion. This region of Serpens contains what is referred to as the Serpens Cloud. It has been cataloged in Herbst, Beckwith, Robberto, 1997 Astrophys. J. This super cloud of dust contains many reflection nebulae, one of which is vdB 123. This is the blue reflection nebula

L'Ecole polytechnique, 1 rue Descartes, Paris 5e. From its creation in 1794, the school, which took the name of Polytechnique in September 1795, was thus clearly defined. She must give her students a solid scientific training, based on mathematics, physics and chemistry, and train them to enter the special schools of the public services of the State, such as the school of application of artillery and genie, the school of mines or that of Ponts et Chaussees. To take over the students judges who were too indisciplinary outside, Napoleon decided to take over them by imposing a military regime on them in 1804. They set them up on the Sainte Genevieve Mountain, in the premises of the College of Navarre and the College of Boncourt. Place they will not leave until 1976.
L'Ecole polytechnique, 1 rue Descartes, Paris 5e. From its creation in 1794, the school, which took the name of Polytechnique in September 1795, was thus clearly defined. She must give her students a solid scientific training, based on mathematics, physics and chemistry, and train them to enter the special schools of the public services of the State, such as the school of application of artillery and genie, the school of mines or that of Ponts et Chaussees. To take over the students judges who were too indisciplinary outside, Napoleon decided to take over them by imposing a military regime on them in 1804. They set them up on the Sainte Genevieve Mountain, in the premises of the College of Navarre and the College of Boncourt. Place they will not leave until 1976.

TEC4622298: L'Ecole polytechnique, 1 rue Descartes, Paris 5e. From its creation in 1794, the school, which took the name of Polytechnique in September 1795, was thus clearly defined. She must give her students a solid scientific training, based on mathematics, physics and chemistry, and train them to enter the special schools of the public services of the State, such as the school of application of artillery and genie, the school of mines or that of Ponts et Chaussees. To take over the students judges who were too indisciplinary outside, Napoleon decided to take over them by imposing a military regime on them in 1804. They set them up on the Sainte Genevieve Mountain, in the premises of the College of Navarre and the College of Boncourt. Place they will not leave until 1976. / Bridgeman Images

ID: TEC4622298

L'Ecole polytechnique, 1 rue Descartes, Paris 5e. From its creation in 1794, the school, which took the name of Polytechnique in September 1795, was thus clearly defined. She must give her students a solid scientific training, based on mathematics, physics and chemistry, and train them to enter the special schools of the public services of the State, such as the school of application of artillery and genie, the school of mines or that of Ponts et Chaussees. To take over the students judges who were too indisciplinary outside, Napoleon decided to take over them by imposing a military regime on them in 1804. They set them up on the Sainte Genevieve Mountain, in the premises of the College of Navarre and the College of Boncourt. Place they will not leave until 1976.

Mel 15 star cluster in the nebula IC 1805 - IC1805 Heart Nebula - Melotte 15 is a cluster of young stars composed of massive OB-type stars. Age about 1.5 million years, this cluster is located 50 years - light in front of the nebula it illuminates. Melotte 15 is an extremely young cluster of massive OB stars with a mean age of only 1.5 million years. The cluster is positioned some 50 light years in front of the nebula it illuminates
Mel 15 star cluster in the nebula IC 1805 - IC1805 Heart Nebula - Melotte 15 is a cluster of young stars composed of massive OB-type stars. Age about 1.5 million years, this cluster is located 50 years - light in front of the nebula it illuminates. Melotte 15 is an extremely young cluster of massive OB stars with a mean age of only 1.5 million years. The cluster is positioned some 50 light years in front of the nebula it illuminates

PIX4622391: Mel 15 star cluster in the nebula IC 1805 - IC1805 Heart Nebula - Melotte 15 is a cluster of young stars composed of massive OB-type stars. Age about 1.5 million years, this cluster is located 50 years - light in front of the nebula it illuminates. Melotte 15 is an extremely young cluster of massive OB stars with a mean age of only 1.5 million years. The cluster is positioned some 50 light years in front of the nebula it illuminates / Bridgeman Images

ID: PIX4622391

Mel 15 star cluster in the nebula IC 1805 - IC1805 Heart Nebula - Melotte 15 is a cluster of young stars composed of massive OB-type stars. Age about 1.5 million years, this cluster is located 50 years - light in front of the nebula it illuminates. Melotte 15 is an extremely young cluster of massive OB stars with a mean age of only 1.5 million years. The cluster is positioned some 50 light years in front of the nebula it illuminates

Bust of bearded man, 15th century (drawing)
Bust of bearded man, 15th century (drawing)

LRI4621895: Bust of bearded man, 15th century (drawing), Pisanello, Antonio (1395-1455) / Bridgeman Images

ID: LRI4621895

Bust of bearded man, 15th century (drawing)

Pisanello, Antonio (1395-1455)

Horse's Head Nebula - The Horsehead nebula in Orion - The Horse's Head Nebula, Barnard 33, is a dark nebula located in front of the IC 434 emission nebula at about 1500 years - light of the Earth in the constellation Orion. Lower left is the reflexion nebula, NGC 2023. The Horsehead nebula is located in the constellation of Orion, slightly below the left - most star of the three that form the Hunter's belt. It is part of a vast molecular cloud of dust and gas that includes the Great Orion Nebula and extends throughout the entire constellation as well. Here we see the Horsehead as it appeared 1,500 years ago, due to distance and the time it takes light to travel
Horse's Head Nebula - The Horsehead nebula in Orion - The Horse's Head Nebula, Barnard 33, is a dark nebula located in front of the IC 434 emission nebula at about 1500 years - light of the Earth in the constellation Orion. Lower left is the reflexion nebula, NGC 2023. The Horsehead nebula is located in the constellation of Orion, slightly below the left - most star of the three that form the Hunter's belt. It is part of a vast molecular cloud of dust and gas that includes the Great Orion Nebula and extends throughout the entire constellation as well. Here we see the Horsehead as it appeared 1,500 years ago, due to distance and the time it takes light to travel

PIX4622102: Horse's Head Nebula - The Horsehead nebula in Orion - The Horse's Head Nebula, Barnard 33, is a dark nebula located in front of the IC 434 emission nebula at about 1500 years - light of the Earth in the constellation Orion. Lower left is the reflexion nebula, NGC 2023. The Horsehead nebula is located in the constellation of Orion, slightly below the left - most star of the three that form the Hunter's belt. It is part of a vast molecular cloud of dust and gas that includes the Great Orion Nebula and extends throughout the entire constellation as well. Here we see the Horsehead as it appeared 1,500 years ago, due to distance and the time it takes light to travel / Bridgeman Images

ID: PIX4622102

Horse's Head Nebula - The Horsehead nebula in Orion - The Horse's Head Nebula, Barnard 33, is a dark nebula located in front of the IC 434 emission nebula at about 1500 years - light of the Earth in the constellation Orion. Lower left is the reflexion nebula, NGC 2023. The Horsehead nebula is located in the constellation of Orion, slightly below the left - most star of the three that form the Hunter's belt. It is part of a vast molecular cloud of dust and gas that includes the Great Orion Nebula and extends throughout the entire constellation as well. Here we see the Horsehead as it appeared 1,500 years ago, due to distance and the time it takes light to travel

Clean site, landscaping in Strasbourgæ (Alsace).
Clean site, landscaping in Strasbourgæ (Alsace).

LBY4619224: Clean site, landscaping in Strasbourgæ (Alsace). / Bridgeman Images

ID: LBY4619224

Clean site, landscaping in Strasbourgæ (Alsace).

Nebulae NGC 3576 and 3603 in Carene. - Star formation regions NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight
Nebulae NGC 3576 and 3603 in Carene. - Star formation regions NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight

PIX4619230: Nebulae NGC 3576 and 3603 in Carene. - Star formation regions NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight / Bridgeman Images

ID: PIX4619230

Nebulae NGC 3576 and 3603 in Carene. - Star formation regions NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight

The tram in Strasbourg (Alsace). Photograhie 04/04/00.
The tram in Strasbourg (Alsace). Photograhie 04/04/00.

LBY4619245: The tram in Strasbourg (Alsace). Photograhie 04/04/00. / Bridgeman Images

ID: LBY4619245

The tram in Strasbourg (Alsace). Photograhie 04/04/00.

Nebula NGC 6334 in Scorpio - Nebula NGC 6334 in Scorpio
Nebula NGC 6334 in Scorpio - Nebula NGC 6334 in Scorpio

PIX4619334: Nebula NGC 6334 in Scorpio - Nebula NGC 6334 in Scorpio / Bridgeman Images

ID: PIX4619334

Nebula NGC 6334 in Scorpio - Nebula NGC 6334 in Scorpio

Tristan and Yseult. Poster for the dramatic poem, 20th century
Tristan and Yseult. Poster for the dramatic poem, 20th century

LRI4619439: Tristan and Yseult. Poster for the dramatic poem, 20th century, Marussig, Guido (1885-1972) / Bridgeman Images

ID: LRI4619439

Tristan and Yseult. Poster for the dramatic poem, 20th century

Marussig, Guido (1885-1972)

Strasbourg station (Bas Rhin, Alsace). Extension, Station Square. Architects Jean Marie Duthilleul and Etienne Tricaud, realisation 2007. Photography 30/07/08.
Strasbourg station (Bas Rhin, Alsace). Extension, Station Square. Architects Jean Marie Duthilleul and Etienne Tricaud, realisation 2007. Photography 30/07/08.

MDA4619533: Strasbourg station (Bas Rhin, Alsace). Extension, Station Square. Architects Jean Marie Duthilleul and Etienne Tricaud, realisation 2007. Photography 30/07/08., Duthilleul, Jean Marie (b.1952) / Bridgeman Images

ID: MDA4619533

Strasbourg station (Bas Rhin, Alsace). Extension, Station Square. Architects Jean Marie Duthilleul and Etienne Tricaud, realisation 2007. Photography 30/07/08.

Duthilleul, Jean Marie (b.1952)

Nebula NGC 6164 - 5 in the Rule - The emission nebula NGC 6164 - 65 - This nebula is located about 4000 years - light from Earth. It is a bipolar nebula around a very hot star at the end of life, the star HD 148937. Image obtained by Siding Spring's 3.9m telescope. Superficially similar to a planetary nebula, NGC 6164 - 5 is in reality a rather unusual object associated with a rather unusual star. The vivid blue central star, known only as HD 148937, is the brightest member of a triple system of stars in orbit around each other. This extremely hot star is loosing mass from its outer layers continuously, but occasionally more vigorous outbursts give rise to the symmetrical shells seen in this picture. The two catalogue numbers, NGC 6164 and 6165, refer to these shells as separate objects
Nebula NGC 6164 - 5 in the Rule - The emission nebula NGC 6164 - 65 - This nebula is located about 4000 years - light from Earth. It is a bipolar nebula around a very hot star at the end of life, the star HD 148937. Image obtained by Siding Spring's 3.9m telescope. Superficially similar to a planetary nebula, NGC 6164 - 5 is in reality a rather unusual object associated with a rather unusual star. The vivid blue central star, known only as HD 148937, is the brightest member of a triple system of stars in orbit around each other. This extremely hot star is loosing mass from its outer layers continuously, but occasionally more vigorous outbursts give rise to the symmetrical shells seen in this picture. The two catalogue numbers, NGC 6164 and 6165, refer to these shells as separate objects

PIX4619235: Nebula NGC 6164 - 5 in the Rule - The emission nebula NGC 6164 - 65 - This nebula is located about 4000 years - light from Earth. It is a bipolar nebula around a very hot star at the end of life, the star HD 148937. Image obtained by Siding Spring's 3.9m telescope. Superficially similar to a planetary nebula, NGC 6164 - 5 is in reality a rather unusual object associated with a rather unusual star. The vivid blue central star, known only as HD 148937, is the brightest member of a triple system of stars in orbit around each other. This extremely hot star is loosing mass from its outer layers continuously, but occasionally more vigorous outbursts give rise to the symmetrical shells seen in this picture. The two catalogue numbers, NGC 6164 and 6165, refer to these shells as separate objects / Bridgeman Images

ID: PIX4619235

Nebula NGC 6164 - 5 in the Rule - The emission nebula NGC 6164 - 65 - This nebula is located about 4000 years - light from Earth. It is a bipolar nebula around a very hot star at the end of life, the star HD 148937. Image obtained by Siding Spring's 3.9m telescope. Superficially similar to a planetary nebula, NGC 6164 - 5 is in reality a rather unusual object associated with a rather unusual star. The vivid blue central star, known only as HD 148937, is the brightest member of a triple system of stars in orbit around each other. This extremely hot star is loosing mass from its outer layers continuously, but occasionally more vigorous outbursts give rise to the symmetrical shells seen in this picture. The two catalogue numbers, NGC 6164 and 6165, refer to these shells as separate objects

The buildings of the former Seegmuller armaments factory in Strasbourg, Port du Rhine (Alsace). Photography 04/07/00.
The buildings of the former Seegmuller armaments factory in Strasbourg, Port du Rhine (Alsace). Photography 04/07/00.

LBY4619252: The buildings of the former Seegmuller armaments factory in Strasbourg, Port du Rhine (Alsace). Photography 04/07/00. / Bridgeman Images

ID: LBY4619252

The buildings of the former Seegmuller armaments factory in Strasbourg, Port du Rhine (Alsace). Photography 04/07/00.

Advertising Poster for Alman Felice, Torino - Milano, Italy
Advertising Poster for Alman Felice, Torino - Milano, Italy

LRI4619390: Advertising Poster for Alman Felice, Torino - Milano, Italy, Carpanetto, Giovanni Battista (1863-1928) / Bridgeman Images

ID: LRI4619390

Advertising Poster for Alman Felice, Torino - Milano, Italy

Carpanetto, Giovanni Battista (1863-1928)

Strasbourg Train Station (Bas Rhin, Alsace). Extension, Station Square. Architects Jean Marie Duthilleul and Etienne Tricaud, realisation 2007. Photography 30/07/08.
Strasbourg Train Station (Bas Rhin, Alsace). Extension, Station Square. Architects Jean Marie Duthilleul and Etienne Tricaud, realisation 2007. Photography 30/07/08.

MDA4619529: Strasbourg Train Station (Bas Rhin, Alsace). Extension, Station Square. Architects Jean Marie Duthilleul and Etienne Tricaud, realisation 2007. Photography 30/07/08., Duthilleul, Jean Marie (b.1952) / Bridgeman Images

ID: MDA4619529

Strasbourg Train Station (Bas Rhin, Alsace). Extension, Station Square. Architects Jean Marie Duthilleul and Etienne Tricaud, realisation 2007. Photography 30/07/08.

Duthilleul, Jean Marie (b.1952)

Corner building, Rue Drouot, Paris 9th.
Corner building, Rue Drouot, Paris 9th.

MDA4618598: Corner building, Rue Drouot, Paris 9th. / Bridgeman Images

ID: MDA4618598

Corner building, Rue Drouot, Paris 9th.


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