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781476 Search Results for Photography

Auvers-sur-Oise : Auberge Ravoux
Auvers-sur-Oise : Auberge Ravoux

MLO2496749: Auvers-sur-Oise : Auberge Ravoux / Bridgeman Images

ID: MLO2496749

Auvers-sur-Oise : Auberge Ravoux

Auvers-sur-Oise : Auberge Ravoux
Auvers-sur-Oise : Auberge Ravoux

MLO2496756: Auvers-sur-Oise : Auberge Ravoux / Bridgeman Images

ID: MLO2496756

Auvers-sur-Oise : Auberge Ravoux

Sculpture by Jean Claude HUG
Sculpture by Jean Claude HUG

BLO2519351: Sculpture by Jean Claude HUG, Hug, Jean-Claude (b.1939) / Bridgeman Images

ID: BLO2519351

Sculpture by Jean Claude HUG

Hug, Jean-Claude (b.1939)

Sculpture by Jean Claude HUG
Sculpture by Jean Claude HUG

BLO2519352: Sculpture by Jean Claude HUG, Hug, Jean-Claude (b.1939) / Bridgeman Images

ID: BLO2519352

Sculpture by Jean Claude HUG

Hug, Jean-Claude (b.1939)

Wim Wenders, 2004 (photo)
Wim Wenders, 2004 (photo)

AGF2531002: Wim Wenders, 2004 (photo) / Bridgeman Images

ID: AGF2531002

Wim Wenders, 2004 (photo)

Thierry Jonquet and Didier Daeninckx
Thierry Jonquet and Didier Daeninckx

MLO2478859: Thierry Jonquet and Didier Daeninckx / Bridgeman Images

ID: MLO2478859

Thierry Jonquet and Didier Daeninckx

Jean Claude Pirotte
Jean Claude Pirotte

MLO2392331: Jean Claude Pirotte / Bridgeman Images

ID: MLO2392331

Jean Claude Pirotte

Tower of the moon or Chand Minar in Daulatabad fort, Aurangabad, Maharashtra, India (photo)
Tower of the moon or Chand Minar in Daulatabad fort, Aurangabad, Maharashtra, India (photo)

DND2561172: Tower of the moon or Chand Minar in Daulatabad fort, Aurangabad, Maharashtra, India (photo) / Bridgeman Images

ID: DND2561172

Tower of the moon or Chand Minar in Daulatabad fort, Aurangabad, Maharashtra, India (photo)

NULL
NULL

COF3863124: NULL / Bridgeman Images

ID: COF3863124

NULL

Children looking at toys, Paris, December 14, 1949 (Christmas) (b/w photo)
Children looking at toys, Paris, December 14, 1949 (Christmas) (b/w photo)

XRA2825211: Children looking at toys, Paris, December 14, 1949 (Christmas) (b/w photo) / Bridgeman Images

ID: XRA2825211

Children looking at toys, Paris, December 14, 1949 (Christmas) (b/w photo)

Kapp Putsch, Berlin, 1920 (b/w photo)
Kapp Putsch, Berlin, 1920 (b/w photo)

SZT2909318: Kapp Putsch, Berlin, 1920 (b/w photo) / Bridgeman Images

ID: SZT2909318

Kapp Putsch, Berlin, 1920 (b/w photo)

Kapp Putsch, Berlin, 1920 (b/w photo)
Kapp Putsch, Berlin, 1920 (b/w photo)

SZT2909325: Kapp Putsch, Berlin, 1920 (b/w photo) / Bridgeman Images

ID: SZT2909325

Kapp Putsch, Berlin, 1920 (b/w photo)

Members of the Bismarck Federation and battle squadrons, Berlin, 1933 (b/w photo)
Members of the Bismarck Federation and battle squadrons, Berlin, 1933 (b/w photo)

SZT2909336: Members of the Bismarck Federation and battle squadrons, Berlin, 1933 (b/w photo) / Bridgeman Images

ID: SZT2909336

Members of the Bismarck Federation and battle squadrons, Berlin, 1933 (b/w photo)

Elly Beinhorn-Rosemeyer, pilot, Germany, 1907 (b/w photo)
Elly Beinhorn-Rosemeyer, pilot, Germany, 1907 (b/w photo)

SZT2909500: Elly Beinhorn-Rosemeyer, pilot, Germany, 1907 (b/w photo) / Bridgeman Images

ID: SZT2909500

Elly Beinhorn-Rosemeyer, pilot, Germany, 1907 (b/w photo)

Elly Beinhorn-Rosemeyer, pilot, Germany, 1907 (b/w photo)
Elly Beinhorn-Rosemeyer, pilot, Germany, 1907 (b/w photo)

SZT2909504: Elly Beinhorn-Rosemeyer, pilot, Germany, 1907 (b/w photo) / Bridgeman Images

ID: SZT2909504

Elly Beinhorn-Rosemeyer, pilot, Germany, 1907 (b/w photo)

The German aviator Elly Beinhorn-Rosemeyer, 1937 (b/w photo)
The German aviator Elly Beinhorn-Rosemeyer, 1937 (b/w photo)

SZT2909488: The German aviator Elly Beinhorn-Rosemeyer, 1937 (b/w photo) / Bridgeman Images

ID: SZT2909488

The German aviator Elly Beinhorn-Rosemeyer, 1937 (b/w photo)

Algerian children (from Arris) having a snack at Matignon, Paris, in presence of Michel Debre, Nafissa Sid Cara and Paul Delouvier, September 13, 1960 (b/w photo)
Algerian children (from Arris) having a snack at Matignon, Paris, in presence of Michel Debre, Nafissa Sid Cara and Paul Delouvier, September 13, 1960 (b/w photo)

XRA2898634: Algerian children (from Arris) having a snack at Matignon, Paris, in presence of Michel Debre, Nafissa Sid Cara and Paul Delouvier, September 13, 1960 (b/w photo) / Bridgeman Images

ID: XRA2898634

Algerian children (from Arris) having a snack at Matignon, Paris, in presence of Michel Debre, Nafissa Sid Cara and Paul Delouvier, September 13, 1960 (b/w photo)

Fritzi Massary (b/w photo)
Fritzi Massary (b/w photo)

SZT2914500: Fritzi Massary (b/w photo) / Bridgeman Images

ID: SZT2914500

Fritzi Massary (b/w photo)

Fritzi Massary (b/w photo)
Fritzi Massary (b/w photo)

SZT2914501: Fritzi Massary (b/w photo) / Bridgeman Images

ID: SZT2914501

Fritzi Massary (b/w photo)

Mary Wigman (b/w photo)
Mary Wigman (b/w photo)

SZT2914507: Mary Wigman (b/w photo) / Bridgeman Images

ID: SZT2914507

Mary Wigman (b/w photo)

Mary Wigman (b/w photo)
Mary Wigman (b/w photo)

SZT2914508: Mary Wigman (b/w photo) / Bridgeman Images

ID: SZT2914508

Mary Wigman (b/w photo)

Mary Wigman (b/w photo)
Mary Wigman (b/w photo)

SZT2914511: Mary Wigman (b/w photo) / Bridgeman Images

ID: SZT2914511

Mary Wigman (b/w photo)

Mary Wigman (b/w photo)
Mary Wigman (b/w photo)

SZT2914515: Mary Wigman (b/w photo) / Bridgeman Images

ID: SZT2914515

Mary Wigman (b/w photo)

View of the area of the locking belt Heiligendamm the G8 summit of 2500 meters height, 2007 (b/w photo)
View of the area of the locking belt Heiligendamm the G8 summit of 2500 meters height, 2007 (b/w photo)

SZT2967312: View of the area of the locking belt Heiligendamm the G8 summit of 2500 meters height, 2007 (b/w photo) / Bridgeman Images

ID: SZT2967312

View of the area of the locking belt Heiligendamm the G8 summit of 2500 meters height, 2007 (b/w photo)

Grand Hotel Heiligendamm with Hohenzollern Castle in Mecklenburg-Vorpommern, 2012 (b/w photo)
Grand Hotel Heiligendamm with Hohenzollern Castle in Mecklenburg-Vorpommern, 2012 (b/w photo)

SZT2967338: Grand Hotel Heiligendamm with Hohenzollern Castle in Mecklenburg-Vorpommern, 2012 (b/w photo) / Bridgeman Images

ID: SZT2967338

Grand Hotel Heiligendamm with Hohenzollern Castle in Mecklenburg-Vorpommern, 2012 (b/w photo)

Matei Visniec
Matei Visniec

MLO2960466: Matei Visniec / Bridgeman Images

ID: MLO2960466

Matei Visniec

The Daimler-Niederrad was constructed under the direction of Gottlieb Daimler by Wilhelm Maybach and was probably the first motorcycle in the world (b/w photo)
The Daimler-Niederrad was constructed under the direction of Gottlieb Daimler by Wilhelm Maybach and was probably the first motorcycle in the world (b/w photo)

SZT2956679: The Daimler-Niederrad was constructed under the direction of Gottlieb Daimler by Wilhelm Maybach and was probably the first motorcycle in the world (b/w photo) / Bridgeman Images

ID: SZT2956679

The Daimler-Niederrad was constructed under the direction of Gottlieb Daimler by Wilhelm Maybach and was probably the first motorcycle in the world (b/w photo)

Karl Maybach, inventor and designer, 1879 (b/w photo)
Karl Maybach, inventor and designer, 1879 (b/w photo)

SZT2956685: Karl Maybach, inventor and designer, 1879 (b/w photo) / Bridgeman Images

ID: SZT2956685

Karl Maybach, inventor and designer, 1879 (b/w photo)

Austro-Hungarian pack-train at the crossing of the Vardar to the Macedonian border, 1916 (b/w photo)
Austro-Hungarian pack-train at the crossing of the Vardar to the Macedonian border, 1916 (b/w photo)

SZT2956696: Austro-Hungarian pack-train at the crossing of the Vardar to the Macedonian border, 1916 (b/w photo) / Bridgeman Images

ID: SZT2956696

Austro-Hungarian pack-train at the crossing of the Vardar to the Macedonian border, 1916 (b/w photo)

Planetary nebula NGC 7027 in the Swan/HST - This NASA Hubble Space Telescope image of planetary nebula NGC 7027 shows remarkable new details of the process by which a star like the Sun dies. New features include: faint, blue, concentric shells surrounding the nebula; an extensive network of red dust clouds throughout the bright inner region; and the hot central white dwarf, visible as a white dot at the center. The nebula is a record of the star's final death throes. Initially the ejection of the star's outer layers, when it was at its red giant stage of evolution, occurred at a low rate and was spherical. The Hubble photo reveals that the initial ejections occurred episodically to produce the concentric shells. This culminated in a vigorous ejection of all of the remaining outer layers, which produced the bright inner regions. At this later stage the ejection was non - spherical, and dense clouds of dust condensed from the ejected material. NGC 7027 is located about 3,000 light - years from Earth in the direction of the summer constellation Cygnus. When a star like the Sun nears the end of its life, it expands to more than 50 times its original diameter, becoming a red giant star. Then its outer layers are ejected into space, exposing the small, extremely hot core of the star, which cools off to become a white dwarf. Although stars like the Sun can live for up to 10 billion years before becoming a red giant and ejecting a nebula, the actual ejection process takes only a few thousand years. The NGC 7027 photograph is a composite of two Hubble images, taken in visible and infrared light, and is shown in “” pseudo - color.
Planetary nebula NGC 7027 in the Swan/HST - This NASA Hubble Space Telescope image of planetary nebula NGC 7027 shows remarkable new details of the process by which a star like the Sun dies. New features include: faint, blue, concentric shells surrounding the nebula; an extensive network of red dust clouds throughout the bright inner region; and the hot central white dwarf, visible as a white dot at the center. The nebula is a record of the star's final death throes. Initially the ejection of the star's outer layers, when it was at its red giant stage of evolution, occurred at a low rate and was spherical. The Hubble photo reveals that the initial ejections occurred episodically to produce the concentric shells. This culminated in a vigorous ejection of all of the remaining outer layers, which produced the bright inner regions. At this later stage the ejection was non - spherical, and dense clouds of dust condensed from the ejected material. NGC 7027 is located about 3,000 light - years from Earth in the direction of the summer constellation Cygnus. When a star like the Sun nears the end of its life, it expands to more than 50 times its original diameter, becoming a red giant star. Then its outer layers are ejected into space, exposing the small, extremely hot core of the star, which cools off to become a white dwarf. Although stars like the Sun can live for up to 10 billion years before becoming a red giant and ejecting a nebula, the actual ejection process takes only a few thousand years. The NGC 7027 photograph is a composite of two Hubble images, taken in visible and infrared light, and is shown in “” pseudo - color.

PIX4623552: Planetary nebula NGC 7027 in the Swan/HST - This NASA Hubble Space Telescope image of planetary nebula NGC 7027 shows remarkable new details of the process by which a star like the Sun dies. New features include: faint, blue, concentric shells surrounding the nebula; an extensive network of red dust clouds throughout the bright inner region; and the hot central white dwarf, visible as a white dot at the center. The nebula is a record of the star's final death throes. Initially the ejection of the star's outer layers, when it was at its red giant stage of evolution, occurred at a low rate and was spherical. The Hubble photo reveals that the initial ejections occurred episodically to produce the concentric shells. This culminated in a vigorous ejection of all of the remaining outer layers, which produced the bright inner regions. At this later stage the ejection was non - spherical, and dense clouds of dust condensed from the ejected material. NGC 7027 is located about 3,000 light - years from Earth in the direction of the summer constellation Cygnus. When a star like the Sun nears the end of its life, it expands to more than 50 times its original diameter, becoming a red giant star. Then its outer layers are ejected into space, exposing the small, extremely hot core of the star, which cools off to become a white dwarf. Although stars like the Sun can live for up to 10 billion years before becoming a red giant and ejecting a nebula, the actual ejection process takes only a few thousand years. The NGC 7027 photograph is a composite of two Hubble images, taken in visible and infrared light, and is shown in “” pseudo - color. / Bridgeman Images

ID: PIX4623552

Planetary nebula NGC 7027 in the Swan/HST - This NASA Hubble Space Telescope image of planetary nebula NGC 7027 shows remarkable new details of the process by which a star like the Sun dies. New features include: faint, blue, concentric shells surrounding the nebula; an extensive network of red dust clouds throughout the bright inner region; and the hot central white dwarf, visible as a white dot at the center. The nebula is a record of the star's final death throes. Initially the ejection of the star's outer layers, when it was at its red giant stage of evolution, occurred at a low rate and was spherical. The Hubble photo reveals that the initial ejections occurred episodically to produce the concentric shells. This culminated in a vigorous ejection of all of the remaining outer layers, which produced the bright inner regions. At this later stage the ejection was non - spherical, and dense clouds of dust condensed from the ejected material. NGC 7027 is located about 3,000 light - year

Planetary nebula IC 418 dans le Lievre/HST - IC 418: The “” Spirograph” Nebula Glowing like a multi - faceted jewel, the planetary nebula IC 418 lies about 2,000 light - years from Earth in the direction of the constellation Lepus. This photograph is from Nasa's Hubble Space Telescope, obtained with the Wide Field Planetary Camera 2. A planetary nebula represents the final stage in the evolution of a star similar to our Sun. The star at the center of IC 418 was a red giant a few thousand years ago, but then ejected its outer layers into space to form the nebula, which has now expanded to a diameter of about 0.1 light - year. The stellar remnant at the center is the hot core of the red giant, from which ultraviolet radiation floods out into the surrounding gas, causing it to fluoresce. Over the next several thousand years, the nebula will gradually disperse into space, and then the star will cool and fade away for billions of years as a white dwarf. Our own Sun is expected to undergo a similar fate, but fortunately this will not occur until some 5 billion years from now. The Hubble image of IC 418 is shown in a false - color representation, based on Wide Field Planetary Camera 2 exposures taken in February and September, 1999 through filters that isolate light from various chemical elements. Red shows emission from ionized nitrogen (the coolest gas in the nebula, located furthest from the hot nucleus), green shows emission from hydrogen, and blue traces the emission from ionized oxygen (the hottest gas, closest to the central star)
Planetary nebula IC 418 dans le Lievre/HST - IC 418: The “” Spirograph” Nebula Glowing like a multi - faceted jewel, the planetary nebula IC 418 lies about 2,000 light - years from Earth in the direction of the constellation Lepus. This photograph is from Nasa's Hubble Space Telescope, obtained with the Wide Field Planetary Camera 2. A planetary nebula represents the final stage in the evolution of a star similar to our Sun. The star at the center of IC 418 was a red giant a few thousand years ago, but then ejected its outer layers into space to form the nebula, which has now expanded to a diameter of about 0.1 light - year. The stellar remnant at the center is the hot core of the red giant, from which ultraviolet radiation floods out into the surrounding gas, causing it to fluoresce. Over the next several thousand years, the nebula will gradually disperse into space, and then the star will cool and fade away for billions of years as a white dwarf. Our own Sun is expected to undergo a similar fate, but fortunately this will not occur until some 5 billion years from now. The Hubble image of IC 418 is shown in a false - color representation, based on Wide Field Planetary Camera 2 exposures taken in February and September, 1999 through filters that isolate light from various chemical elements. Red shows emission from ionized nitrogen (the coolest gas in the nebula, located furthest from the hot nucleus), green shows emission from hydrogen, and blue traces the emission from ionized oxygen (the hottest gas, closest to the central star)

PIX4623677: Planetary nebula IC 418 dans le Lievre/HST - IC 418: The “” Spirograph” Nebula Glowing like a multi - faceted jewel, the planetary nebula IC 418 lies about 2,000 light - years from Earth in the direction of the constellation Lepus. This photograph is from Nasa's Hubble Space Telescope, obtained with the Wide Field Planetary Camera 2. A planetary nebula represents the final stage in the evolution of a star similar to our Sun. The star at the center of IC 418 was a red giant a few thousand years ago, but then ejected its outer layers into space to form the nebula, which has now expanded to a diameter of about 0.1 light - year. The stellar remnant at the center is the hot core of the red giant, from which ultraviolet radiation floods out into the surrounding gas, causing it to fluoresce. Over the next several thousand years, the nebula will gradually disperse into space, and then the star will cool and fade away for billions of years as a white dwarf. Our own Sun is expected to undergo a similar fate, but fortunately this will not occur until some 5 billion years from now. The Hubble image of IC 418 is shown in a false - color representation, based on Wide Field Planetary Camera 2 exposures taken in February and September, 1999 through filters that isolate light from various chemical elements. Red shows emission from ionized nitrogen (the coolest gas in the nebula, located furthest from the hot nucleus), green shows emission from hydrogen, and blue traces the emission from ionized oxygen (the hottest gas, closest to the central star) / Bridgeman Images

ID: PIX4623677

Planetary nebula IC 418 dans le Lievre/HST - IC 418: The “” Spirograph” Nebula Glowing like a multi - faceted jewel, the planetary nebula IC 418 lies about 2,000 light - years from Earth in the direction of the constellation Lepus. This photograph is from Nasa's Hubble Space Telescope, obtained with the Wide Field Planetary Camera 2. A planetary nebula represents the final stage in the evolution of a star similar to our Sun. The star at the center of IC 418 was a red giant a few thousand years ago, but then ejected its outer layers into space to form the nebula, which has now expanded to a diameter of about 0.1 light - year. The stellar remnant at the center is the hot core of the red giant, from which ultraviolet radiation floods out into the surrounding gas, causing it to fluoresce. Over the next several thousand years, the nebula will gradually disperse into space, and then the star will cool and fade away for billions of years as a white dwarf. Our own Sun is expected to undergo a

Sardar Hardit Singh Malik, Indian ambassador in France, here in Paris on April 18, 1949 (b/w photo)
Sardar Hardit Singh Malik, Indian ambassador in France, here in Paris on April 18, 1949 (b/w photo)

XRA2661012: Sardar Hardit Singh Malik, Indian ambassador in France, here in Paris on April 18, 1949 (b/w photo) / Bridgeman Images

ID: XRA2661012

Sardar Hardit Singh Malik, Indian ambassador in France, here in Paris on April 18, 1949 (b/w photo)

Sardar Hardit Singh Malik, Indian ambassador in France, here in Paris on April 18, 1949 (b/w photo)
Sardar Hardit Singh Malik, Indian ambassador in France, here in Paris on April 18, 1949 (b/w photo)

XRA2661013: Sardar Hardit Singh Malik, Indian ambassador in France, here in Paris on April 18, 1949 (b/w photo) / Bridgeman Images

ID: XRA2661013

Sardar Hardit Singh Malik, Indian ambassador in France, here in Paris on April 18, 1949 (b/w photo)

Visit of Queen Juliana of Netherlands in Paris, May 24, 1950 : here at Paris city hall (b:w photo)
Visit of Queen Juliana of Netherlands in Paris, May 24, 1950 : here at Paris city hall (b:w photo)

XRA2674659: Visit of Queen Juliana of Netherlands in Paris, May 24, 1950 : here at Paris city hall (b:w photo) / Bridgeman Images

ID: XRA2674659

Visit of Queen Juliana of Netherlands in Paris, May 24, 1950 : here at Paris city hall (b:w photo)

XRA2673262: "Prix de l'Arc de Triomphe", Longchamp racecourse, Paris, October 9, 1960 : the winner the jockey Garcia on the horse Puissant Chef followed by Hautain (b/w photo) / Bridgeman Images

ID: XRA2673262

"Prix de l'Arc de Triomphe", Longchamp racecourse, Paris, October 9, 1960 : the winner the jockey Garcia on the horse Puissant Chef followed by Hautain (b/w photo)

Georges Chelon (b/w photo)
Georges Chelon (b/w photo)

XRA2693549: Georges Chelon (b/w photo) / Bridgeman Images

ID: XRA2693549

Georges Chelon (b/w photo)


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