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781408 Search Results for Photography

Pont du Gard/Gard/Languedoc/France
Pont du Gard/Gard/Languedoc/France

HFE5951736: Pont du Gard/Gard/Languedoc/France / Bridgeman Images

Hulk Hogan, undated (photo)
Hulk Hogan, undated (photo)

EVC5956468: Hulk Hogan, undated (photo) / Bridgeman Images

Ingrid Rosselini Isabella Rosselini mom Pia Lindstrom, 1989 (photo)
Ingrid Rosselini Isabella Rosselini mom Pia Lindstrom, 1989 (photo)

EVC5956501: Ingrid Rosselini Isabella Rosselini mom Pia Lindstrom, 1989 (photo) / Bridgeman Images

Nakata Ryo
Nakata Ryo

WAN3895572: Nakata Ryo / Bridgeman Images

GENTLEMAN'S AGREEMENT, from left, Ransom Sherman, Celeste Holm, Gregory Peck, 1947
GENTLEMAN'S AGREEMENT, from left, Ransom Sherman, Celeste Holm, Gregory Peck, 1947

EVC5971414: GENTLEMAN'S AGREEMENT, from left, Ransom Sherman, Celeste Holm, Gregory Peck, 1947 / Bridgeman Images

THE CRUSADES, from left: assistant director George Hippard watches as director Cecil B. DeMille instructs the actors for a crowd scene on set, 1935
THE CRUSADES, from left: assistant director George Hippard watches as director Cecil B. DeMille instructs the actors for a crowd scene on set, 1935

EVC5968335: THE CRUSADES, from left: assistant director George Hippard watches as director Cecil B. DeMille instructs the actors for a crowd scene on set, 1935 / Bridgeman Images

Pope John Paul II's family house, Poland, 2000 (photo)
Pope John Paul II's family house, Poland, 2000 (photo)

MEP6100541: Pope John Paul II's family house, Poland, 2000 (photo) / Bridgeman Images

Oryx - Oryx - Oryx gazelle (Oryx gazella), or gemsbok. Kalahari, South Africa. Gemsbok or gemsbuck (Oryx gazella). Kalahari, Republic of south africa
Oryx - Oryx - Oryx gazelle (Oryx gazella), or gemsbok. Kalahari, South Africa. Gemsbok or gemsbuck (Oryx gazella). Kalahari, Republic of south africa

PIX4677742: Oryx - Oryx - Oryx gazelle (Oryx gazella), or gemsbok. Kalahari, South Africa. Gemsbok or gemsbuck (Oryx gazella). Kalahari, Republic of south africa / Bridgeman Images

The Moon above the Earth's atmosphere - Gibbous moon above the atmosphere - The moon observed from the International Space Station (ISS). A gibbous moon above Earth's atmosphere is featured in this view, photographed by an Expedition 22 crewmember on the International Space Station (ISS)
The Moon above the Earth's atmosphere - Gibbous moon above the atmosphere - The moon observed from the International Space Station (ISS). A gibbous moon above Earth's atmosphere is featured in this view, photographed by an Expedition 22 crewmember on the International Space Station (ISS)

PIX4675211: The Moon above the Earth's atmosphere - Gibbous moon above the atmosphere - The moon observed from the International Space Station (ISS). A gibbous moon above Earth's atmosphere is featured in this view, photographed by an Expedition 22 crewmember on the International Space Station (ISS) / Bridgeman Images

Sunrise seen from shuttle Endeavour 09/1992 - Sunrise in earth atmosphere 09/1992 - Sunrise in atmosphere seen from shuttle Endeavour on 18 September 1992. Sunrise in earth atmosphere seen from space shuttle Endeavour on September 18, 1992
Sunrise seen from shuttle Endeavour 09/1992 - Sunrise in earth atmosphere 09/1992 - Sunrise in atmosphere seen from shuttle Endeavour on 18 September 1992. Sunrise in earth atmosphere seen from space shuttle Endeavour on September 18, 1992

PIX4675308: Sunrise seen from shuttle Endeavour 09/1992 - Sunrise in earth atmosphere 09/1992 - Sunrise in atmosphere seen from shuttle Endeavour on 18 September 1992. Sunrise in earth atmosphere seen from space shuttle Endeavour on September 18, 1992 / Bridgeman Images

The air metro station at Barbes Rochechouart station in Paris 75018.
The air metro station at Barbes Rochechouart station in Paris 75018.

TEC4645678: The air metro station at Barbes Rochechouart station in Paris 75018. / Bridgeman Images

Old building in Paris 75018 from rue Livingstone. Photography 10/04/06.
Old building in Paris 75018 from rue Livingstone. Photography 10/04/06.

TEC4645501: Old building in Paris 75018 from rue Livingstone. Photography 10/04/06. / Bridgeman Images

Rehabilitation of social housing units, HBM group, 54-56 quai du Point du Jour, rue de Seine et Emile Duclaux, avenue Pierre Grenier a Boulogne Billancourt (Hauts de Seine). Construction 1932, architects Joseph Bassompierre (1871-1950), Paul de Rutte (1871-1943) and Paul Sirvin (1891-1977). Rehabilitation from 1992 to 1996 by Patrick Magendie. This complex consisted of approximately 1,000 houses on a plot of 27,500 square metres. The accommodation consists of a majority of three rooms and four rooms. The common rooms are open to the alcove kitchen, following which is installed the laundry room with sink, wash basin and shower!
Rehabilitation of social housing units, HBM group, 54-56 quai du Point du Jour, rue de Seine et Emile Duclaux, avenue Pierre Grenier a Boulogne Billancourt (Hauts de Seine). Construction 1932, architects Joseph Bassompierre (1871-1950), Paul de Rutte (1871-1943) and Paul Sirvin (1891-1977). Rehabilitation from 1992 to 1996 by Patrick Magendie. This complex consisted of approximately 1,000 houses on a plot of 27,500 square metres. The accommodation consists of a majority of three rooms and four rooms. The common rooms are open to the alcove kitchen, following which is installed the laundry room with sink, wash basin and shower!

MDA4673140: Rehabilitation of social housing units, HBM group, 54-56 quai du Point du Jour, rue de Seine et Emile Duclaux, avenue Pierre Grenier a Boulogne Billancourt (Hauts de Seine). Construction 1932, architects Joseph Bassompierre (1871-1950), Paul de Rutte (1871-1943) and Paul Sirvin (1891-1977). Rehabilitation from 1992 to 1996 by Patrick Magendie. This complex consisted of approximately 1,000 houses on a plot of 27,500 square metres. The accommodation consists of a majority of three rooms and four rooms. The common rooms are open to the alcove kitchen, following which is installed the laundry room with sink, wash basin and shower! / Bridgeman Images

Rehabilitation of social housing units, HBM group, 54-56 quai du Point du Jour, rue de Seine et Emile Duclaux, avenue Pierre Grenier a Boulogne Billancourt (Hauts de Seine). Construction 1932, architects Joseph Bassompierre (1871-1950), Paul de Rutte (1871-1943) and Paul Sirvin (1891-1977). Rehabilitation from 1992 to 1996 by Patrick Magendie. This complex consisted of approximately 1,000 houses on a plot of 27,500 square metres. The accommodation consists of a majority of three rooms and four rooms. The common rooms are open to the alcove kitchen, following which is installed the laundry room with sink, wash basin and shower!
Rehabilitation of social housing units, HBM group, 54-56 quai du Point du Jour, rue de Seine et Emile Duclaux, avenue Pierre Grenier a Boulogne Billancourt (Hauts de Seine). Construction 1932, architects Joseph Bassompierre (1871-1950), Paul de Rutte (1871-1943) and Paul Sirvin (1891-1977). Rehabilitation from 1992 to 1996 by Patrick Magendie. This complex consisted of approximately 1,000 houses on a plot of 27,500 square metres. The accommodation consists of a majority of three rooms and four rooms. The common rooms are open to the alcove kitchen, following which is installed the laundry room with sink, wash basin and shower!

MDA4673155: Rehabilitation of social housing units, HBM group, 54-56 quai du Point du Jour, rue de Seine et Emile Duclaux, avenue Pierre Grenier a Boulogne Billancourt (Hauts de Seine). Construction 1932, architects Joseph Bassompierre (1871-1950), Paul de Rutte (1871-1943) and Paul Sirvin (1891-1977). Rehabilitation from 1992 to 1996 by Patrick Magendie. This complex consisted of approximately 1,000 houses on a plot of 27,500 square metres. The accommodation consists of a majority of three rooms and four rooms. The common rooms are open to the alcove kitchen, following which is installed the laundry room with sink, wash basin and shower! / Bridgeman Images

Earth clouds and atmosphere - Earth clouds and atmosphere - Clouds and Earth atmosphere seen from the International Space Station (ISS) in February 2010. Clouds and terrestrial astmosphere as seen by the International Space Station (ISS). February 2010
Earth clouds and atmosphere - Earth clouds and atmosphere - Clouds and Earth atmosphere seen from the International Space Station (ISS) in February 2010. Clouds and terrestrial astmosphere as seen by the International Space Station (ISS). February 2010

PIX4674967: Earth clouds and atmosphere - Earth clouds and atmosphere - Clouds and Earth atmosphere seen from the International Space Station (ISS) in February 2010. Clouds and terrestrial astmosphere as seen by the International Space Station (ISS). February 2010 / Bridgeman Images

Parc de Sceaux in the Hauts de Seine.
Parc de Sceaux in the Hauts de Seine.

TEC4651515: Parc de Sceaux in the Hauts de Seine. / Bridgeman Images

Courbevoie in the Hauts de Seine. Photography 01/10/95.
Courbevoie in the Hauts de Seine. Photography 01/10/95.

TEC4651568: Courbevoie in the Hauts de Seine. Photography 01/10/95. / Bridgeman Images

Solar panel on the Forum esplanade in Barcelona, Spain. Photography 18/02/08
Solar panel on the Forum esplanade in Barcelona, Spain. Photography 18/02/08

TEC4680224: Solar panel on the Forum esplanade in Barcelona, Spain. Photography 18/02/08 / Bridgeman Images

Egyptian antiquite: partial view of the hypostyl room with columns decorated with the representation of the goddess Hathor. Temple of Hathor, Denderah, Egypt
Egyptian antiquite: partial view of the hypostyl room with columns decorated with the representation of the goddess Hathor. Temple of Hathor, Denderah, Egypt

LRI4681752: Egyptian antiquite: partial view of the hypostyl room with columns decorated with the representation of the goddess Hathor. Temple of Hathor, Denderah, Egypt, Egyptian Ptolemaic Period (332-30 BC) / Bridgeman Images

Etruscan civilization: Symposium accessory in silver ceramic from a tomb of Poggio Sala, Italy 4th century BC Dim 23 cm (accessory for the symposium) 4th century BC Florence, Museo Archeologico, inv 77651
Etruscan civilization: Symposium accessory in silver ceramic from a tomb of Poggio Sala, Italy 4th century BC Dim 23 cm (accessory for the symposium) 4th century BC Florence, Museo Archeologico, inv 77651

LRI4689215: Etruscan civilization: Symposium accessory in silver ceramic from a tomb of Poggio Sala, Italy 4th century BC Dim 23 cm (accessory for the symposium) 4th century BC Florence, Museo Archeologico, inv 77651, Etruscan, (4th century BC) / Bridgeman Images

House “” Chaume 01”” in Bourg Achard (Bourg-Achard) in Haute-Normandie (Haute Normandie), France. Architecture of CO-BE Architecture and Landscape, 2007. Photography 10/06/07
House “” Chaume 01”” in Bourg Achard (Bourg-Achard) in Haute-Normandie (Haute Normandie), France. Architecture of CO-BE Architecture and Landscape, 2007. Photography 10/06/07

LBY4685289: House “” Chaume 01”” in Bourg Achard (Bourg-Achard) in Haute-Normandie (Haute Normandie), France. Architecture of CO-BE Architecture and Landscape, 2007. Photography 10/06/07 / Bridgeman Images

Nebula IC 2220 in the Carene - A mass - loss star in IC 2220 - This nebula is illuminated by a giant red star, the star HD 65670. Image obtained by Siding Spring's 3.9m telescope. The bright, supergiant star at the centre of this nebula is known only by its catalog designation, HD 65750. The nebulosity around the star is the result of light reflected by dust surrounding it. The dust is thought to consist mainly of particles of silica condensed from material which the star is losing from its distended surface at a fairly steady rate. The rate of mass loss is much higher than in normal stars and is sufficient to produce the reflection nebula IC 2220. The stellar nature of the central object is revealed by the four diffraction spikes extending from it. These are artifacts due to structures within the telescope. The light from the star has also produced the annular halation ring (a photographic artefact) that ornaments the nebula. These features, real or otherwise, have provoked the name 'Toby Jug' for this nebula, after the ornamental English drinking vessel or beer mug
Nebula IC 2220 in the Carene - A mass - loss star in IC 2220 - This nebula is illuminated by a giant red star, the star HD 65670. Image obtained by Siding Spring's 3.9m telescope. The bright, supergiant star at the centre of this nebula is known only by its catalog designation, HD 65750. The nebulosity around the star is the result of light reflected by dust surrounding it. The dust is thought to consist mainly of particles of silica condensed from material which the star is losing from its distended surface at a fairly steady rate. The rate of mass loss is much higher than in normal stars and is sufficient to produce the reflection nebula IC 2220. The stellar nature of the central object is revealed by the four diffraction spikes extending from it. These are artifacts due to structures within the telescope. The light from the star has also produced the annular halation ring (a photographic artefact) that ornaments the nebula. These features, real or otherwise, have provoked the name 'Toby Jug' for this nebula, after the ornamental English drinking vessel or beer mug

PIX4622497: Nebula IC 2220 in the Carene - A mass - loss star in IC 2220 - This nebula is illuminated by a giant red star, the star HD 65670. Image obtained by Siding Spring's 3.9m telescope. The bright, supergiant star at the centre of this nebula is known only by its catalog designation, HD 65750. The nebulosity around the star is the result of light reflected by dust surrounding it. The dust is thought to consist mainly of particles of silica condensed from material which the star is losing from its distended surface at a fairly steady rate. The rate of mass loss is much higher than in normal stars and is sufficient to produce the reflection nebula IC 2220. The stellar nature of the central object is revealed by the four diffraction spikes extending from it. These are artifacts due to structures within the telescope. The light from the star has also produced the annular halation ring (a photographic artefact) that ornaments the nebula. These features, real or otherwise, have provoked the name 'Toby Jug' for this nebula, after the ornamental English drinking vessel or beer mug / Bridgeman Images

Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula M57 in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained by the Hubble Space Telescope. This close - up, visible - light view by Nasa's Hubble Space Telescope reveals new details of the Ring Nebula. The object is tilted towards Earth so that astronomers see the ring face - on. The Hubble observations reveal that the nebula's shape is more complicated than astronomers thought. The blue gas in the nebula's center is actually a football - shaped structure that pierces the red doughnut - shaped material. Hubble also uncovers the detailed structure of the dark, irregular knots of dense gas embedded along the inner rim of the ring. The knots look like spokes in a bicycle. The Hubble images have allowed the research team to match up the knots with the spikes of light around the bright, main ring, which are a shadow effect. The Ring Nebula is a well - known planetary nebula, the glowing remains of a Sun - like star. The tiny white dot in the center of the nebula is the star's hot core, called a white dwarf. The nebula is about 2,000 light - years away in the constellation Lyra. The structure measures roughly one light - year across. The Hubble observations were taken Sept. 19, 2011, by the Wide Field Camera 3. In the image, the deep blue color in the center represents helium; the cyan color of the inner ring is the glow of hydrogen and oxygen; and the reddish color of the outer ring is from nitrogen and sulfur
Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula M57 in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained by the Hubble Space Telescope. This close - up, visible - light view by Nasa's Hubble Space Telescope reveals new details of the Ring Nebula. The object is tilted towards Earth so that astronomers see the ring face - on. The Hubble observations reveal that the nebula's shape is more complicated than astronomers thought. The blue gas in the nebula's center is actually a football - shaped structure that pierces the red doughnut - shaped material. Hubble also uncovers the detailed structure of the dark, irregular knots of dense gas embedded along the inner rim of the ring. The knots look like spokes in a bicycle. The Hubble images have allowed the research team to match up the knots with the spikes of light around the bright, main ring, which are a shadow effect. The Ring Nebula is a well - known planetary nebula, the glowing remains of a Sun - like star. The tiny white dot in the center of the nebula is the star's hot core, called a white dwarf. The nebula is about 2,000 light - years away in the constellation Lyra. The structure measures roughly one light - year across. The Hubble observations were taken Sept. 19, 2011, by the Wide Field Camera 3. In the image, the deep blue color in the center represents helium; the cyan color of the inner ring is the glow of hydrogen and oxygen; and the reddish color of the outer ring is from nitrogen and sulfur

PIX4623343: Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula M57 in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained by the Hubble Space Telescope. This close - up, visible - light view by Nasa's Hubble Space Telescope reveals new details of the Ring Nebula. The object is tilted towards Earth so that astronomers see the ring face - on. The Hubble observations reveal that the nebula's shape is more complicated than astronomers thought. The blue gas in the nebula's center is actually a football - shaped structure that pierces the red doughnut - shaped material. Hubble also uncovers the detailed structure of the dark, irregular knots of dense gas embedded along the inner rim of the ring. The knots look like spokes in a bicycle. The Hubble images have allowed the research team to match up the knots with the spikes of light around the bright, main ring, which are a shadow effect. The Ring Nebula is a well - known planetary nebula, the glowing remains of a Sun - like star. The tiny white dot in the center of the nebula is the star's hot core, called a white dwarf. The nebula is about 2,000 light - years away in the constellation Lyra. The structure measures roughly one light - year across. The Hubble observations were taken Sept. 19, 2011, by the Wide Field Camera 3. In the image, the deep blue color in the center represents helium; the cyan color of the inner ring is the glow of hydrogen and oxygen; and the reddish color of the outer ring is from nitrogen and sulfur / Bridgeman Images

Planetary nebula M57 (NGC 6720) in Lyra - M57 (NGC 6720) planetary nebula in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. With a magnitude of 9.0, this nebula is easily observed with a small telescope. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Composite image obtained by different telescopes. The Ring Nebula, M57, is the most famous example of a planetary nebula. Located about 2,000 light years away, it has an apparent diameter of 1 arc minute and a real diameter of about one light year. At magnitude 9.0 its high surface brightness makes it an easy object, even from the city and even with small telescopes. Planetary nebula are shells of gas shed by stars late in their life cycles after using up all of their nuclear fuel. The star then ejects a significant portion of its mass in a gaseous shell, which is illuminated by its extremely hot central star, which is just the core left from the original star. The star at the center of the Ring nebula has a surface temperature of 216,000 degrees Farenheit or 120,000 degrees Celsius. Our own star, the Sun, is expected to undergo the same process in a couple of billion years. Planetary nebulae do not last long at all in cosmic terms, the shell of gas expands and diffuse, becoming invisible, and the star turns into a white dwarf. Composite image from three data sources: HST, LBT, Subaru
Planetary nebula M57 (NGC 6720) in Lyra - M57 (NGC 6720) planetary nebula in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. With a magnitude of 9.0, this nebula is easily observed with a small telescope. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Composite image obtained by different telescopes. The Ring Nebula, M57, is the most famous example of a planetary nebula. Located about 2,000 light years away, it has an apparent diameter of 1 arc minute and a real diameter of about one light year. At magnitude 9.0 its high surface brightness makes it an easy object, even from the city and even with small telescopes. Planetary nebula are shells of gas shed by stars late in their life cycles after using up all of their nuclear fuel. The star then ejects a significant portion of its mass in a gaseous shell, which is illuminated by its extremely hot central star, which is just the core left from the original star. The star at the center of the Ring nebula has a surface temperature of 216,000 degrees Farenheit or 120,000 degrees Celsius. Our own star, the Sun, is expected to undergo the same process in a couple of billion years. Planetary nebulae do not last long at all in cosmic terms, the shell of gas expands and diffuse, becoming invisible, and the star turns into a white dwarf. Composite image from three data sources: HST, LBT, Subaru

PIX4623359: Planetary nebula M57 (NGC 6720) in Lyra - M57 (NGC 6720) planetary nebula in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. With a magnitude of 9.0, this nebula is easily observed with a small telescope. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Composite image obtained by different telescopes. The Ring Nebula, M57, is the most famous example of a planetary nebula. Located about 2,000 light years away, it has an apparent diameter of 1 arc minute and a real diameter of about one light year. At magnitude 9.0 its high surface brightness makes it an easy object, even from the city and even with small telescopes. Planetary nebula are shells of gas shed by stars late in their life cycles after using up all of their nuclear fuel. The star then ejects a significant portion of its mass in a gaseous shell, which is illuminated by its extremely hot central star, which is just the core left from the original star. The star at the center of the Ring nebula has a surface temperature of 216,000 degrees Farenheit or 120,000 degrees Celsius. Our own star, the Sun, is expected to undergo the same process in a couple of billion years. Planetary nebulae do not last long at all in cosmic terms, the shell of gas expands and diffuse, becoming invisible, and the star turns into a white dwarf. Composite image from three data sources: HST, LBT, Subaru / Bridgeman Images

Avenue Pierre Larousse in Malakoff in the Hauts de Seine.
Avenue Pierre Larousse in Malakoff in the Hauts de Seine.

TEC4651042: Avenue Pierre Larousse in Malakoff in the Hauts de Seine. / Bridgeman Images

Church of the Holy Spirit, Avenue Daumesnil in Paris. Architect Paul Tournon (1881-1964), 1935.
Church of the Holy Spirit, Avenue Daumesnil in Paris. Architect Paul Tournon (1881-1964), 1935.

TEC4627842: Church of the Holy Spirit, Avenue Daumesnil in Paris. Architect Paul Tournon (1881-1964), 1935. / Bridgeman Images

The city of Quimper in Brittany, Cathedrale Saint Corentin (Saint Corentin). Photography 11/08/09.
The city of Quimper in Brittany, Cathedrale Saint Corentin (Saint Corentin). Photography 11/08/09.

TEC4634585: The city of Quimper in Brittany, Cathedrale Saint Corentin (Saint Corentin). Photography 11/08/09. / Bridgeman Images

The city of Quimper in Brittany, Cathedrale Saint Corentin (Saint Corentin). Photography 11/08/09.
The city of Quimper in Brittany, Cathedrale Saint Corentin (Saint Corentin). Photography 11/08/09.

TEC4634627: The city of Quimper in Brittany, Cathedrale Saint Corentin (Saint Corentin). Photography 11/08/09. / Bridgeman Images

Nacreous clouds - Nacreous clouds - PSC for Polar Stratospheric Cloud observed in Norway. Nacreous cloud (or PSC for polar stratospheric cloud) seen in Norway
Nacreous clouds - Nacreous clouds - PSC for Polar Stratospheric Cloud observed in Norway. Nacreous cloud (or PSC for polar stratospheric cloud) seen in Norway

PIX4634025: Nacreous clouds - Nacreous clouds - PSC for Polar Stratospheric Cloud observed in Norway. Nacreous cloud (or PSC for polar stratospheric cloud) seen in Norway / Bridgeman Images

Nacreous clouds - Nacreous clouds - PSC for Polar Stratospheric Cloud observed in Norway. Nacreous cloud (or PSC for polar stratospheric cloud) seen in Norway
Nacreous clouds - Nacreous clouds - PSC for Polar Stratospheric Cloud observed in Norway. Nacreous cloud (or PSC for polar stratospheric cloud) seen in Norway

PIX4634061: Nacreous clouds - Nacreous clouds - PSC for Polar Stratospheric Cloud observed in Norway. Nacreous cloud (or PSC for polar stratospheric cloud) seen in Norway / Bridgeman Images

Maison d'Eileen Gray in Roquebrune Cap Martin (Roquebrune-Cap-Martin or Roquebrune Cap-Martin), Alpes-Maritimes (Alpes Maritimes), Provence-Alpes-Cote d'Azur (Provence Alpes Cote d'Azur). Architecture by Jean Badovici, 1929. Photography 04/02/10
Maison d'Eileen Gray in Roquebrune Cap Martin (Roquebrune-Cap-Martin or Roquebrune Cap-Martin), Alpes-Maritimes (Alpes Maritimes), Provence-Alpes-Cote d'Azur (Provence Alpes Cote d'Azur). Architecture by Jean Badovici, 1929. Photography 04/02/10

OMG4658110: Maison d'Eileen Gray in Roquebrune Cap Martin (Roquebrune-Cap-Martin or Roquebrune Cap-Martin), Alpes-Maritimes (Alpes Maritimes), Provence-Alpes-Cote d'Azur (Provence Alpes Cote d'Azur). Architecture by Jean Badovici, 1929. Photography 04/02/10 / Bridgeman Images

La rue de Tour in Paris 16th.
La rue de Tour in Paris 16th.

TEC4624369: La rue de Tour in Paris 16th. / Bridgeman Images

The museum of Louvre-Lens Louvre-Lens - 2012, Kazuyo Sejima and Ryue Nishizawa - Sanaa Agency -
The museum of Louvre-Lens Louvre-Lens - 2012, Kazuyo Sejima and Ryue Nishizawa - Sanaa Agency -

LBY4698157: The museum of Louvre-Lens Louvre-Lens - 2012, Kazuyo Sejima and Ryue Nishizawa - Sanaa Agency - / Bridgeman Images

La Galerie du Temps du Musee du Louvre-Lens - 2012, Kazuyo Sejima and Ryue Nishizawa - Sanaa Agency -
La Galerie du Temps du Musee du Louvre-Lens - 2012, Kazuyo Sejima and Ryue Nishizawa - Sanaa Agency -

MDA4698206: La Galerie du Temps du Musee du Louvre-Lens - 2012, Kazuyo Sejima and Ryue Nishizawa - Sanaa Agency - / Bridgeman Images

The Oberlin Museum in Waldersbach (Bas Rhin). Architect Frederic Jung, 2003. Photography 18/05/06.
The Oberlin Museum in Waldersbach (Bas Rhin). Architect Frederic Jung, 2003. Photography 18/05/06.

MDA4696067: The Oberlin Museum in Waldersbach (Bas Rhin). Architect Frederic Jung, 2003. Photography 18/05/06. / Bridgeman Images

Rehabilitation of the Musee Saint-Pierre in Lyon. Architecture by Philippe Dubois and Jean-Michel Wilmotte, 1992-1998. Photography 1994
Rehabilitation of the Musee Saint-Pierre in Lyon. Architecture by Philippe Dubois and Jean-Michel Wilmotte, 1992-1998. Photography 1994

TEC4707061: Rehabilitation of the Musee Saint-Pierre in Lyon. Architecture by Philippe Dubois and Jean-Michel Wilmotte, 1992-1998. Photography 1994, Wilmotte, Jean-Michel (b.1948) & Dubois, Philippe / Bridgeman Images


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