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Nebula of the Lagoon (M8) in the Sagittair
Nebula of the Lagoon (M8) in the Sagittair

PIX4619635: Nebula of the Lagoon (M8) in the Sagittair / Bridgeman Images

ID: PIX4619635

Nebula of the Lagoon (M8) in the Sagittair

Nebulae M20 - M8 and NGC 6559 in Sagittair
Nebulae M20 - M8 and NGC 6559 in Sagittair

PIX4619746: Nebulae M20 - M8 and NGC 6559 in Sagittair / Bridgeman Images

ID: PIX4619746

Nebulae M20 - M8 and NGC 6559 in Sagittair

Nebulae M20-M8 and NGC 6559 in Sagittarius - Nebulae NGC 6559 Lagoon and Trifid in Sagittarius: View of nebulae of the Lagoon (M8/NGC 6523), bottom, Trifide (M20), top, and NGC 6559 (left). Located in Sagittarius, these nebulae are about 5000 light years away from Earth. Lagoon nebula (bottom), NGC 6559 (bottom left), Trifid (top right) with top left the open cluster M21. These nebulae are located 5000 light years away in Sagittarius constellation.
Nebulae M20-M8 and NGC 6559 in Sagittarius - Nebulae NGC 6559 Lagoon and Trifid in Sagittarius: View of nebulae of the Lagoon (M8/NGC 6523), bottom, Trifide (M20), top, and NGC 6559 (left). Located in Sagittarius, these nebulae are about 5000 light years away from Earth. Lagoon nebula (bottom), NGC 6559 (bottom left), Trifid (top right) with top left the open cluster M21. These nebulae are located 5000 light years away in Sagittarius constellation.

PIX4619790: Nebulae M20-M8 and NGC 6559 in Sagittarius - Nebulae NGC 6559 Lagoon and Trifid in Sagittarius: View of nebulae of the Lagoon (M8/NGC 6523), bottom, Trifide (M20), top, and NGC 6559 (left). Located in Sagittarius, these nebulae are about 5000 light years away from Earth. Lagoon nebula (bottom), NGC 6559 (bottom left), Trifid (top right) with top left the open cluster M21. These nebulae are located 5000 light years away in Sagittarius constellation. / Bridgeman Images

ID: PIX4619790

Nebulae M20-M8 and NGC 6559 in Sagittarius - Nebulae NGC 6559 Lagoon and Trifid in Sagittarius: View of nebulae of the Lagoon (M8/NGC 6523), bottom, Trifide (M20), top, and NGC 6559 (left). Located in Sagittarius, these nebulae are about 5000 light years away from Earth. Lagoon nebula (bottom), NGC 6559 (bottom left), Trifid (top right) with top left the open cluster M21. These nebulae are located 5000 light years away in Sagittarius constellation.

History of France in the Middle Ages: Tomb of the King of France Louis XI (1423-1483), 1905 (illustration)
History of France in the Middle Ages: Tomb of the King of France Louis XI (1423-1483), 1905 (illustration)

JLJ4619669: History of France in the Middle Ages: Tomb of the King of France Louis XI (1423-1483), 1905 (illustration), Job, pseudonym for Onfray de Breville, Jacques (1858-1931) / Bridgeman Images

ID: JLJ4619669

History of France in the Middle Ages: Tomb of the King of France Louis XI (1423-1483), 1905 (illustration)

Job, pseudonym for Onfray de Breville, Jacques (1858-1931)

Nebulae M8 and NGC 6559 in Sagittarius - Nebulae M8 and NGC 6559 in Sagittarius - View of nebulae of the Lagoon (M - 8/ngc 6523), on the right, and of NGC 6559 (left). Located in Sagittarius, these nebulae are about 5000 light years away from Earth
Nebulae M8 and NGC 6559 in Sagittarius - Nebulae M8 and NGC 6559 in Sagittarius - View of nebulae of the Lagoon (M - 8/ngc 6523), on the right, and of NGC 6559 (left). Located in Sagittarius, these nebulae are about 5000 light years away from Earth

PIX4619732: Nebulae M8 and NGC 6559 in Sagittarius - Nebulae M8 and NGC 6559 in Sagittarius - View of nebulae of the Lagoon (M - 8/ngc 6523), on the right, and of NGC 6559 (left). Located in Sagittarius, these nebulae are about 5000 light years away from Earth / Bridgeman Images

ID: PIX4619732

Nebulae M8 and NGC 6559 in Sagittarius - Nebulae M8 and NGC 6559 in Sagittarius - View of nebulae of the Lagoon (M - 8/ngc 6523), on the right, and of NGC 6559 (left). Located in Sagittarius, these nebulae are about 5000 light years away from Earth

Nebulae M20 - M8 and NGC 6559 in Sagittarius - Nebulae M20 - M8 and NGC 6559 in Sagittarius - View of nebulae of the Lagoon (M - 8/ngc 6523), bottom, Trifide (M20), top, and NGC 6559 (left). Located in Sagittarius, these nebulae are about 5000 light years away from Earth
Nebulae M20 - M8 and NGC 6559 in Sagittarius - Nebulae M20 - M8 and NGC 6559 in Sagittarius - View of nebulae of the Lagoon (M - 8/ngc 6523), bottom, Trifide (M20), top, and NGC 6559 (left). Located in Sagittarius, these nebulae are about 5000 light years away from Earth

PIX4619744: Nebulae M20 - M8 and NGC 6559 in Sagittarius - Nebulae M20 - M8 and NGC 6559 in Sagittarius - View of nebulae of the Lagoon (M - 8/ngc 6523), bottom, Trifide (M20), top, and NGC 6559 (left). Located in Sagittarius, these nebulae are about 5000 light years away from Earth / Bridgeman Images

ID: PIX4619744

Nebulae M20 - M8 and NGC 6559 in Sagittarius - Nebulae M20 - M8 and NGC 6559 in Sagittarius - View of nebulae of the Lagoon (M - 8/ngc 6523), bottom, Trifide (M20), top, and NGC 6559 (left). Located in Sagittarius, these nebulae are about 5000 light years away from Earth

Panoramic view of the Mitte district in Berlin Mitte district - Berlinae -
Panoramic view of the Mitte district in Berlin Mitte district - Berlinae -

TEC4619756: Panoramic view of the Mitte district in Berlin Mitte district - Berlinae - / Bridgeman Images

ID: TEC4619756

Panoramic view of the Mitte district in Berlin Mitte district - Berlinae -

Nebula NGC 6334 in the Scorpion - The 'reddened' nebulosity of NGC 6334 - The nebula NGC 6334 is located about 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The star - forming nebula NGC 6334 shows no evidence of a blue component in their colour - indeed, the blue - light plate used in these 3 - colour pictures had no nebulous image at all - nor is there any obvious sign of the bright blue stars normally found in these objects. They are excellent examples of the phenomenon known as 'interstellar reddening', the selective removal of blue light by minute particles of dust in the line of sight. This accounts for both the ruddy hue and apparent absence of blue stars. The hot stars are present but only some of the red part of their light is seen so they are not conspicuous. This nebula is quite nearby (5500 light years) but located close to the Galactic plane and are buried in the dust of the Milky Way. Careful measurement of the colour of stars associated with the nebula indicate that they are dimmed by a factor of about 10 in the green part of the spectrum, much more in the blue, but relatively little at red wavelengths. Some care has been taken to ensure that these images are as close to true - colour as possible
Nebula NGC 6334 in the Scorpion - The 'reddened' nebulosity of NGC 6334 - The nebula NGC 6334 is located about 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The star - forming nebula NGC 6334 shows no evidence of a blue component in their colour - indeed, the blue - light plate used in these 3 - colour pictures had no nebulous image at all - nor is there any obvious sign of the bright blue stars normally found in these objects. They are excellent examples of the phenomenon known as 'interstellar reddening', the selective removal of blue light by minute particles of dust in the line of sight. This accounts for both the ruddy hue and apparent absence of blue stars. The hot stars are present but only some of the red part of their light is seen so they are not conspicuous. This nebula is quite nearby (5500 light years) but located close to the Galactic plane and are buried in the dust of the Milky Way. Careful measurement of the colour of stars associated with the nebula indicate that they are dimmed by a factor of about 10 in the green part of the spectrum, much more in the blue, but relatively little at red wavelengths. Some care has been taken to ensure that these images are as close to true - colour as possible

PIX4619360: Nebula NGC 6334 in the Scorpion - The 'reddened' nebulosity of NGC 6334 - The nebula NGC 6334 is located about 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The star - forming nebula NGC 6334 shows no evidence of a blue component in their colour - indeed, the blue - light plate used in these 3 - colour pictures had no nebulous image at all - nor is there any obvious sign of the bright blue stars normally found in these objects. They are excellent examples of the phenomenon known as 'interstellar reddening', the selective removal of blue light by minute particles of dust in the line of sight. This accounts for both the ruddy hue and apparent absence of blue stars. The hot stars are present but only some of the red part of their light is seen so they are not conspicuous. This nebula is quite nearby (5500 light years) but located close to the Galactic plane and are buried in the dust of the Milky Way. Careful measurement of the colour of stars associated with the nebula indicate that they are dimmed by a factor of about 10 in the green part of the spectrum, much more in the blue, but relatively little at red wavelengths. Some care has been taken to ensure that these images are as close to true - colour as possible / Bridgeman Images

ID: PIX4619360

Nebula NGC 6334 in the Scorpion - The 'reddened' nebulosity of NGC 6334 - The nebula NGC 6334 is located about 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The star - forming nebula NGC 6334 shows no evidence of a blue component in their colour - indeed, the blue - light plate used in these 3 - colour pictures had no nebulous image at all - nor is there any obvious sign of the bright blue stars normally found in these objects. They are excellent examples of the phenomenon known as 'interstellar reddening', the selective removal of blue light by minute particles of dust in the line of sight. This accounts for both the ruddy hue and apparent absence of blue stars. The hot stars are present but only some of the red part of their light is seen so they are not conspicuous. This nebula is quite nearby (5500 light years) but located close to the Galactic plane and are buried in the dust of the Milky Way. Careful measurement of the colour

Entrée of Pius VII to Paris carries Saint Denis on the day of the sacre of Napoleon, December 2, 1804 (watercolour)
Entrée of Pius VII to Paris carries Saint Denis on the day of the sacre of Napoleon, December 2, 1804 (watercolour)

JLJ4619396: Entrée of Pius VII to Paris carries Saint Denis on the day of the sacre of Napoleon, December 2, 1804 (watercolour), Leleu, Jean Francois (1729-1807) / Bridgeman Images

ID: JLJ4619396

Entrée of Pius VII to Paris carries Saint Denis on the day of the sacre of Napoleon, December 2, 1804 (watercolour)

Leleu, Jean Francois (1729-1807)

Nebula NGC 6357 in Scorpio - Nebula NGC 6357 in Scorpio
Nebula NGC 6357 in Scorpio - Nebula NGC 6357 in Scorpio

PIX4619403: Nebula NGC 6357 in Scorpio - Nebula NGC 6357 in Scorpio / Bridgeman Images

ID: PIX4619403

Nebula NGC 6357 in Scorpio - Nebula NGC 6357 in Scorpio

Trifide nebula (M20) in Sagittarius. - View of the Trifide nebula (M20/ngc 6514) located in the constellation of Sagittarius between 5000 and 10,000 years - light of the Earth
Trifide nebula (M20) in Sagittarius. - View of the Trifide nebula (M20/ngc 6514) located in the constellation of Sagittarius between 5000 and 10,000 years - light of the Earth

PIX4619461: Trifide nebula (M20) in Sagittarius. - View of the Trifide nebula (M20/ngc 6514) located in the constellation of Sagittarius between 5000 and 10,000 years - light of the Earth / Bridgeman Images

ID: PIX4619461

Trifide nebula (M20) in Sagittarius. - View of the Trifide nebula (M20/ngc 6514) located in the constellation of Sagittarius between 5000 and 10,000 years - light of the Earth

Anatomy and surgical boards: crane box, c.1345 (miniature)
Anatomy and surgical boards: crane box, c.1345 (miniature)

JLJ4619554: Anatomy and surgical boards: crane box, c.1345 (miniature), Vigevano da Pavia, Guido da (c.1280-c.1349) / Bridgeman Images

ID: JLJ4619554

Anatomy and surgical boards: crane box, c.1345 (miniature)

Vigevano da Pavia, Guido da (c.1280-c.1349)

Map of the Molucca Archipelago in East Indonesia. Geographic map, 17th century (gouache and lead mine)
Map of the Molucca Archipelago in East Indonesia. Geographic map, 17th century (gouache and lead mine)

JLJ4619573: Map of the Molucca Archipelago in East Indonesia. Geographic map, 17th century (gouache and lead mine), Doetechum, Jan van (17th century) / Bridgeman Images

ID: JLJ4619573

Map of the Molucca Archipelago in East Indonesia. Geographic map, 17th century (gouache and lead mine)

Doetechum, Jan van (17th century)

Lagoon Nebula (M8) - Infrared image of the Lagoon nebula obtained by MSX satellite. The nebula of the Lagoon is located in the constellation Sagittarius at a distance of about 5000 years - light
Lagoon Nebula (M8) - Infrared image of the Lagoon nebula obtained by MSX satellite. The nebula of the Lagoon is located in the constellation Sagittarius at a distance of about 5000 years - light

PIX4619703: Lagoon Nebula (M8) - Infrared image of the Lagoon nebula obtained by MSX satellite. The nebula of the Lagoon is located in the constellation Sagittarius at a distance of about 5000 years - light / Bridgeman Images

ID: PIX4619703

Lagoon Nebula (M8) - Infrared image of the Lagoon nebula obtained by MSX satellite. The nebula of the Lagoon is located in the constellation Sagittarius at a distance of about 5000 years - light

Birth of Louis (then King of France Louis XI (1423-1483), 1905 (illustration)
Birth of Louis (then King of France Louis XI (1423-1483), 1905 (illustration)

JLJ4619887: Birth of Louis (then King of France Louis XI (1423-1483), 1905 (illustration), Job, pseudonym for Onfray de Breville, Jacques (1858-1931) / Bridgeman Images

ID: JLJ4619887

Birth of Louis (then King of France Louis XI (1423-1483), 1905 (illustration)

Job, pseudonym for Onfray de Breville, Jacques (1858-1931)

Store des Westens (KaDeWe), Tauentzienstasse 21/24, Schoneberg in Berlin (Germany). Construction 1906-1907, architect Johann Emil Schaudt (1871-1957). Photography 2003.
Store des Westens (KaDeWe), Tauentzienstasse 21/24, Schoneberg in Berlin (Germany). Construction 1906-1907, architect Johann Emil Schaudt (1871-1957). Photography 2003.

TEC4619852: Store des Westens (KaDeWe), Tauentzienstasse 21/24, Schoneberg in Berlin (Germany). Construction 1906-1907, architect Johann Emil Schaudt (1871-1957). Photography 2003. / Bridgeman Images

ID: TEC4619852

Store des Westens (KaDeWe), Tauentzienstasse 21/24, Schoneberg in Berlin (Germany). Construction 1906-1907, architect Johann Emil Schaudt (1871-1957). Photography 2003.

The Bodes Museum on the island of the Musees in Berlin (Germany).
The Bodes Museum on the island of the Musees in Berlin (Germany).

TEC4619962: The Bodes Museum on the island of the Musees in Berlin (Germany). / Bridgeman Images

ID: TEC4619962

The Bodes Museum on the island of the Musees in Berlin (Germany).

Eagle Nebula (IC 4703) and M16 star cluster in the Snake - The Eagle nebula in Serpens - The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 7000 light years distant
Eagle Nebula (IC 4703) and M16 star cluster in the Snake - The Eagle nebula in Serpens - The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 7000 light years distant

PIX4620019: Eagle Nebula (IC 4703) and M16 star cluster in the Snake - The Eagle nebula in Serpens - The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 7000 light years distant / Bridgeman Images

ID: PIX4620019

Eagle Nebula (IC 4703) and M16 star cluster in the Snake - The Eagle nebula in Serpens - The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 7000 light years distant

Eagle Nebula (IC 4703) and star cluster M16 in the Snake - M16 (NGC 6611) is lying some 7,000 light years distant in the constellation Serpens, close to the borders to Scutum and Sagittarius 12.5” RC, F6, RRGB = 60:10:20
Eagle Nebula (IC 4703) and star cluster M16 in the Snake - M16 (NGC 6611) is lying some 7,000 light years distant in the constellation Serpens, close to the borders to Scutum and Sagittarius 12.5” RC, F6, RRGB = 60:10:20

PIX4619923: Eagle Nebula (IC 4703) and star cluster M16 in the Snake - M16 (NGC 6611) is lying some 7,000 light years distant in the constellation Serpens, close to the borders to Scutum and Sagittarius 12.5” RC, F6, RRGB = 60:10:20 / Bridgeman Images

ID: PIX4619923

Eagle Nebula (IC 4703) and star cluster M16 in the Snake - M16 (NGC 6611) is lying some 7,000 light years distant in the constellation Serpens, close to the borders to Scutum and Sagittarius 12.5” RC, F6, RRGB = 60:10:20

Capriccio antico, 1906 (poster)
Capriccio antico, 1906 (poster)

LRI4619966: Capriccio antico, 1906 (poster), Lambertini, Ludovico (1876-1912) / Bridgeman Images

ID: LRI4619966

Capriccio antico, 1906 (poster)

Lambertini, Ludovico (1876-1912)

Omega nebula (M17) in Sagittarius - The Omega Nebula (M17) in Sagittarius - View of the Omega nebula (M17/ngc 6618) located in the constellation Sagittarius at a distance of 5700 light years
Omega nebula (M17) in Sagittarius - The Omega Nebula (M17) in Sagittarius - View of the Omega nebula (M17/ngc 6618) located in the constellation Sagittarius at a distance of 5700 light years

PIX4620086: Omega nebula (M17) in Sagittarius - The Omega Nebula (M17) in Sagittarius - View of the Omega nebula (M17/ngc 6618) located in the constellation Sagittarius at a distance of 5700 light years / Bridgeman Images

ID: PIX4620086

Omega nebula (M17) in Sagittarius - The Omega Nebula (M17) in Sagittarius - View of the Omega nebula (M17/ngc 6618) located in the constellation Sagittarius at a distance of 5700 light years

Eagle Nebula (IC 4703) and M16 star cluster in the Snake - M16, The Eagle Nebula in Serpens - The M16 star cluster is a cluster of young stars from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Image obtained by combining light through 3 different filters that highlight oxygen, hydrogen, and sulfur. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 7000 light years distant. Issue - line image presented here in false color
Eagle Nebula (IC 4703) and M16 star cluster in the Snake - M16, The Eagle Nebula in Serpens - The M16 star cluster is a cluster of young stars from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Image obtained by combining light through 3 different filters that highlight oxygen, hydrogen, and sulfur. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 7000 light years distant. Issue - line image presented here in false color

PIX4620021: Eagle Nebula (IC 4703) and M16 star cluster in the Snake - M16, The Eagle Nebula in Serpens - The M16 star cluster is a cluster of young stars from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Image obtained by combining light through 3 different filters that highlight oxygen, hydrogen, and sulfur. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 7000 light years distant. Issue - line image presented here in false color / Bridgeman Images

ID: PIX4620021

Eagle Nebula (IC 4703) and M16 star cluster in the Snake - M16, The Eagle Nebula in Serpens - The M16 star cluster is a cluster of young stars from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Image obtained by combining light through 3 different filters that highlight oxygen, hydrogen, and sulfur. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and a

Berlin TV Tower (Fernsehturm), Alexander Platz, Mitte Quarter in Berlin (Germany). Architecteæ Urban Construction Office Schweizer Tscheschner and Schulz, construction 1965-1969. Photography 10/08/03.
Berlin TV Tower (Fernsehturm), Alexander Platz, Mitte Quarter in Berlin (Germany). Architecteæ Urban Construction Office Schweizer Tscheschner and Schulz, construction 1965-1969. Photography 10/08/03.

TEC4620113: Berlin TV Tower (Fernsehturm), Alexander Platz, Mitte Quarter in Berlin (Germany). Architecteæ Urban Construction Office Schweizer Tscheschner and Schulz, construction 1965-1969. Photography 10/08/03. / Bridgeman Images

ID: TEC4620113

Berlin TV Tower (Fernsehturm), Alexander Platz, Mitte Quarter in Berlin (Germany). Architecteæ Urban Construction Office Schweizer Tscheschner and Schulz, construction 1965-1969. Photography 10/08/03.

Television Tower (Fernsehturm), Mitte Quarter in Berlin (Germany). Realisation of the Schweizer Tscheschner and Schulz Urban Construction Office, 1965-1969. Photography 10/08/03.
Television Tower (Fernsehturm), Mitte Quarter in Berlin (Germany). Realisation of the Schweizer Tscheschner and Schulz Urban Construction Office, 1965-1969. Photography 10/08/03.

TEC4620128: Television Tower (Fernsehturm), Mitte Quarter in Berlin (Germany). Realisation of the Schweizer Tscheschner and Schulz Urban Construction Office, 1965-1969. Photography 10/08/03. / Bridgeman Images

ID: TEC4620128

Television Tower (Fernsehturm), Mitte Quarter in Berlin (Germany). Realisation of the Schweizer Tscheschner and Schulz Urban Construction Office, 1965-1969. Photography 10/08/03.

Hotel Adlon, Unter den Linden 75-77 in Berlin (Germany). This hotel, built in 1907, was partially destroyed during the Second World War and rebuilt in 1995-1997 by Patzschke Klotz & Partner. Photography 10/08/03.
Hotel Adlon, Unter den Linden 75-77 in Berlin (Germany). This hotel, built in 1907, was partially destroyed during the Second World War and rebuilt in 1995-1997 by Patzschke Klotz & Partner. Photography 10/08/03.

TEC4620150: Hotel Adlon, Unter den Linden 75-77 in Berlin (Germany). This hotel, built in 1907, was partially destroyed during the Second World War and rebuilt in 1995-1997 by Patzschke Klotz & Partner. Photography 10/08/03. / Bridgeman Images

ID: TEC4620150

Hotel Adlon, Unter den Linden 75-77 in Berlin (Germany). This hotel, built in 1907, was partially destroyed during the Second World War and rebuilt in 1995-1997 by Patzschke Klotz & Partner. Photography 10/08/03.

Wittenbergplatz metro station, Schoneberg district in Berlin (Germany).Architect Alfred Grenander (1863-1931), construction 1911-1913. First underground metro station in Berlin, on the first electric line. Built in reference to the classical buildings of the 18th century. Photography 2003.
Wittenbergplatz metro station, Schoneberg district in Berlin (Germany).Architect Alfred Grenander (1863-1931), construction 1911-1913. First underground metro station in Berlin, on the first electric line. Built in reference to the classical buildings of the 18th century. Photography 2003.

TEC4619849: Wittenbergplatz metro station, Schoneberg district in Berlin (Germany).Architect Alfred Grenander (1863-1931), construction 1911-1913. First underground metro station in Berlin, on the first electric line. Built in reference to the classical buildings of the 18th century. Photography 2003. / Bridgeman Images

ID: TEC4619849

Wittenbergplatz metro station, Schoneberg district in Berlin (Germany).Architect Alfred Grenander (1863-1931), construction 1911-1913. First underground metro station in Berlin, on the first electric line. Built in reference to the classical buildings of the 18th century. Photography 2003.

Portico of the former Anhalter Bahnhof (station), Askanischer Platz, in the district of Kreutzberg in Berlinae (Germany). Architect Franz Schwechten, 1876-1880. Phototoraphie 2003.
Portico of the former Anhalter Bahnhof (station), Askanischer Platz, in the district of Kreutzberg in Berlinae (Germany). Architect Franz Schwechten, 1876-1880. Phototoraphie 2003.

TEC4619876: Portico of the former Anhalter Bahnhof (station), Askanischer Platz, in the district of Kreutzberg in Berlinae (Germany). Architect Franz Schwechten, 1876-1880. Phototoraphie 2003. / Bridgeman Images

ID: TEC4619876

Portico of the former Anhalter Bahnhof (station), Askanischer Platz, in the district of Kreutzberg in Berlinae (Germany). Architect Franz Schwechten, 1876-1880. Phototoraphie 2003.

Nebulae NGC 6589 - 90 in Sagittarius - Nebulosity in Sagittarius, NGC 6589 - 90 - Located in Sagittarius, the reflexion nebulae NGC 6589 - 90 are located at a distance of about 5900 light years from Earth. Image obtained with a telescope 61 cm in diameter. The two bright blue clouds are NGC 6589 and NGC 6590. Image taken with a 24 - inch telescope
Nebulae NGC 6589 - 90 in Sagittarius - Nebulosity in Sagittarius, NGC 6589 - 90 - Located in Sagittarius, the reflexion nebulae NGC 6589 - 90 are located at a distance of about 5900 light years from Earth. Image obtained with a telescope 61 cm in diameter. The two bright blue clouds are NGC 6589 and NGC 6590. Image taken with a 24 - inch telescope

PIX4619908: Nebulae NGC 6589 - 90 in Sagittarius - Nebulosity in Sagittarius, NGC 6589 - 90 - Located in Sagittarius, the reflexion nebulae NGC 6589 - 90 are located at a distance of about 5900 light years from Earth. Image obtained with a telescope 61 cm in diameter. The two bright blue clouds are NGC 6589 and NGC 6590. Image taken with a 24 - inch telescope / Bridgeman Images

ID: PIX4619908

Nebulae NGC 6589 - 90 in Sagittarius - Nebulosity in Sagittarius, NGC 6589 - 90 - Located in Sagittarius, the reflexion nebulae NGC 6589 - 90 are located at a distance of about 5900 light years from Earth. Image obtained with a telescope 61 cm in diameter. The two bright blue clouds are NGC 6589 and NGC 6590. Image taken with a 24 - inch telescope

Portrait en pied du general Jean Andoche Junot (Jean-Andoche) (1771-1813), 19th century (oil on canvas)
Portrait en pied du general Jean Andoche Junot (Jean-Andoche) (1771-1813), 19th century (oil on canvas)

JLJ4620013: Portrait en pied du general Jean Andoche Junot (Jean-Andoche) (1771-1813), 19th century (oil on canvas), Raverat, vincent Nicolas (1801-1865) / Bridgeman Images

ID: JLJ4620013

Portrait en pied du general Jean Andoche Junot (Jean-Andoche) (1771-1813), 19th century (oil on canvas)

Raverat, vincent Nicolas (1801-1865)

Nebulas M16 and M17 in Sagittarius - Nebulas M16 and M17 in Sagittarius - The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. The Omega nebula (M17/NGC 6618), on the right, is located at a distance of 5500 light years. Nebulas M16 (IC 4703) at left, and M17 (NGC 6618) at right in Sagittarius
Nebulas M16 and M17 in Sagittarius - Nebulas M16 and M17 in Sagittarius - The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. The Omega nebula (M17/NGC 6618), on the right, is located at a distance of 5500 light years. Nebulas M16 (IC 4703) at left, and M17 (NGC 6618) at right in Sagittarius

PIX4620092: Nebulas M16 and M17 in Sagittarius - Nebulas M16 and M17 in Sagittarius - The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. The Omega nebula (M17/NGC 6618), on the right, is located at a distance of 5500 light years. Nebulas M16 (IC 4703) at left, and M17 (NGC 6618) at right in Sagittarius / Bridgeman Images

ID: PIX4620092

Nebulas M16 and M17 in Sagittarius - Nebulas M16 and M17 in Sagittarius - The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. The Omega nebula (M17/NGC 6618), on the right, is located at a distance of 5500 light years. Nebulas M16 (IC 4703) at left, and M17 (NGC 6618) at right in Sagittarius

Centre de la nebula Omega (M17) by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls of the hollow cloud shine primarily in the blue, green, and red light emitted by excited atoms of hydrogen, nitrogen, oxygen, and sulfur. Particularly striking is the rose - like feature, seen to the right of center, which glows in the red light emitted by hydrogen and sulfur. ACS made this observation on April 1 and 2, 2002. The color image is constructed from four separate images taken in these filters: blue, near infrared, hydrogen alpha, and doubly ionized oxygen
Centre de la nebula Omega (M17) by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls of the hollow cloud shine primarily in the blue, green, and red light emitted by excited atoms of hydrogen, nitrogen, oxygen, and sulfur. Particularly striking is the rose - like feature, seen to the right of center, which glows in the red light emitted by hydrogen and sulfur. ACS made this observation on April 1 and 2, 2002. The color image is constructed from four separate images taken in these filters: blue, near infrared, hydrogen alpha, and doubly ionized oxygen

PIX4620159: Centre de la nebula Omega (M17) by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls of the hollow cloud shine primarily in the blue, green, and red light emitted by excited atoms of hydrogen, nitrogen, oxygen, and sulfur. Particularly striking is the rose - like feature, seen to the right of center, which glows in the red light emitted by hydrogen and sulfur. ACS made this observation on April 1 and 2, 2002. The color image is constructed from four separate images taken in these filters: blue, near infrared, hydrogen alpha, and doubly ionized oxygen / Bridgeman Images

ID: PIX4620159

Centre de la nebula Omega (M17) by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls of the hollow cloud shin

The Cathedrale Saint Hedwidge, Bebelplatz in Berlin (Germany). Construction 1747-1773, architects Jean Legeay and Johann Boumann.
The Cathedrale Saint Hedwidge, Bebelplatz in Berlin (Germany). Construction 1747-1773, architects Jean Legeay and Johann Boumann.

TEC4620175: The Cathedrale Saint Hedwidge, Bebelplatz in Berlin (Germany). Construction 1747-1773, architects Jean Legeay and Johann Boumann. / Bridgeman Images

ID: TEC4620175

The Cathedrale Saint Hedwidge, Bebelplatz in Berlin (Germany). Construction 1747-1773, architects Jean Legeay and Johann Boumann.

Nebula VDB 143 in Cephee - Nebula VDB 143 in Cepheus - VDB 143 is a nebula by reflexion. Other objects visible in this field are LBN 504, Cederblad 194, LDN 1199. Nebula reflection. Other objects visible are LBN 504, Cederblad 194, LDN 1199
Nebula VDB 143 in Cephee - Nebula VDB 143 in Cepheus - VDB 143 is a nebula by reflexion. Other objects visible in this field are LBN 504, Cederblad 194, LDN 1199. Nebula reflection. Other objects visible are LBN 504, Cederblad 194, LDN 1199

PIX4621776: Nebula VDB 143 in Cephee - Nebula VDB 143 in Cepheus - VDB 143 is a nebula by reflexion. Other objects visible in this field are LBN 504, Cederblad 194, LDN 1199. Nebula reflection. Other objects visible are LBN 504, Cederblad 194, LDN 1199 / Bridgeman Images

ID: PIX4621776

Nebula VDB 143 in Cephee - Nebula VDB 143 in Cepheus - VDB 143 is a nebula by reflexion. Other objects visible in this field are LBN 504, Cederblad 194, LDN 1199. Nebula reflection. Other objects visible are LBN 504, Cederblad 194, LDN 1199

Dark nebula and T star - Tauri in the Swan - Dark nebula and T - Tauri Star in Cygnus - Dark nebula LDN 981 with at its extremite (at the top of the picture) the variable star T - Tauri V1331 Cygni. V1331 Cyg is a variable T - Tauri star located at the tip (top of image) of a long dust filament linking it to the dark cloud LDN 981
Dark nebula and T star - Tauri in the Swan - Dark nebula and T - Tauri Star in Cygnus - Dark nebula LDN 981 with at its extremite (at the top of the picture) the variable star T - Tauri V1331 Cygni. V1331 Cyg is a variable T - Tauri star located at the tip (top of image) of a long dust filament linking it to the dark cloud LDN 981

PIX4621785: Dark nebula and T star - Tauri in the Swan - Dark nebula and T - Tauri Star in Cygnus - Dark nebula LDN 981 with at its extremite (at the top of the picture) the variable star T - Tauri V1331 Cygni. V1331 Cyg is a variable T - Tauri star located at the tip (top of image) of a long dust filament linking it to the dark cloud LDN 981 / Bridgeman Images

ID: PIX4621785

Dark nebula and T star - Tauri in the Swan - Dark nebula and T - Tauri Star in Cygnus - Dark nebula LDN 981 with at its extremite (at the top of the picture) the variable star T - Tauri V1331 Cygni. V1331 Cyg is a variable T - Tauri star located at the tip (top of image) of a long dust filament linking it to the dark cloud LDN 981

Portrait of Hyppolite of Bethune (1603-1665), 17th century (oil on canvas)
Portrait of Hyppolite of Bethune (1603-1665), 17th century (oil on canvas)

JLJ4621853: Portrait of Hyppolite of Bethune (1603-1665), 17th century (oil on canvas), French School, (17th century) / Bridgeman Images

ID: JLJ4621853

Portrait of Hyppolite of Bethune (1603-1665), 17th century (oil on canvas)

French School, (17th century)

Gamma Star Cassiopeia, nebulae IC 59 and IC 6
Gamma Star Cassiopeia, nebulae IC 59 and IC 6

PIX4621819: Gamma Star Cassiopeia, nebulae IC 59 and IC 6 / Bridgeman Images

ID: PIX4621819

Gamma Star Cassiopeia, nebulae IC 59 and IC 6


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