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The Higher School of Fine Arts of Valenciennes (North, North Pas de Calais region). Architect Louis Paillard, 2006.
The Higher School of Fine Arts of Valenciennes (North, North Pas de Calais region). Architect Louis Paillard, 2006.

LBY4560024: The Higher School of Fine Arts of Valenciennes (North, North Pas de Calais region). Architect Louis Paillard, 2006., Paillard, Louis (fl.2006-2008) / Bridgeman Images

The National Conservatory of Dance and Music at La Villette, 209 avenue Jean Jaures, Paris 19th arrondissement. Architect Christian de Portzamparc, 1990.
The National Conservatory of Dance and Music at La Villette, 209 avenue Jean Jaures, Paris 19th arrondissement. Architect Christian de Portzamparc, 1990.

TEC4560089: The National Conservatory of Dance and Music at La Villette, 209 avenue Jean Jaures, Paris 19th arrondissement. Architect Christian de Portzamparc, 1990., Portzamparc, de Christian (b.1944) / Bridgeman Images

The school of Hallue in Saint-Gratien (Somme). Architects Nathalie Hebert and Pierre Louis Fossard, 2006.
The school of Hallue in Saint-Gratien (Somme). Architects Nathalie Hebert and Pierre Louis Fossard, 2006.

MDA4560138: The school of Hallue in Saint-Gratien (Somme). Architects Nathalie Hebert and Pierre Louis Fossard, 2006., Hebert, Nathalie & Fossard, Pierre Louis (21st century) / Bridgeman Images

The school of Hallue in Saint-Gratien (Somme). Architects Nathalie Hebert and Pierre Louis Fossard, 2006.
The school of Hallue in Saint-Gratien (Somme). Architects Nathalie Hebert and Pierre Louis Fossard, 2006.

MDA4560155: The school of Hallue in Saint-Gratien (Somme). Architects Nathalie Hebert and Pierre Louis Fossard, 2006., Hebert, Nathalie & Fossard, Pierre Louis (21st century) / Bridgeman Images

Mediatheque de l'IRCAM, Place Igor Stravinsky, Paris 4th arrondissement. Architect Atelier Canal, 1996.
Mediatheque de l'IRCAM, Place Igor Stravinsky, Paris 4th arrondissement. Architect Atelier Canal, 1996.

MDA4560048: Mediatheque de l'IRCAM, Place Igor Stravinsky, Paris 4th arrondissement. Architect Atelier Canal, 1996., Architecture Canal (f.20th century) / Bridgeman Images

Comete Hale - Bopp - Comet Hale - Bopp C/1995 - Comete Hale - Bopp seen on April 2, 1997, one day after his passage to the perihelie. The Hyades cluster is visible at the top left, then to the right, the Pleiades, Persee, Andromede and Cassiopee. Mercury lies on the mountains at the bottom left of the picture. Comet Hale - Bopp is seen here on April 2, 1997, one day after Perihelion. This is a wide angle shot with the Hyades on the far upper left, then the Pleaides, Perseus, Andromeda and Cassiopeia. Mercury is setting just over the mountains at lower left. Cassel Observatory, New Buffalo, PA, US
Comete Hale - Bopp - Comet Hale - Bopp C/1995 - Comete Hale - Bopp seen on April 2, 1997, one day after his passage to the perihelie. The Hyades cluster is visible at the top left, then to the right, the Pleiades, Persee, Andromede and Cassiopee. Mercury lies on the mountains at the bottom left of the picture. Comet Hale - Bopp is seen here on April 2, 1997, one day after Perihelion. This is a wide angle shot with the Hyades on the far upper left, then the Pleaides, Perseus, Andromeda and Cassiopeia. Mercury is setting just over the mountains at lower left. Cassel Observatory, New Buffalo, PA, US

PIX4569594: Comete Hale - Bopp - Comet Hale - Bopp C/1995 - Comete Hale - Bopp seen on April 2, 1997, one day after his passage to the perihelie. The Hyades cluster is visible at the top left, then to the right, the Pleiades, Persee, Andromede and Cassiopee. Mercury lies on the mountains at the bottom left of the picture. Comet Hale - Bopp is seen here on April 2, 1997, one day after Perihelion. This is a wide angle shot with the Hyades on the far upper left, then the Pleaides, Perseus, Andromeda and Cassiopeia. Mercury is setting just over the mountains at lower left. Cassel Observatory, New Buffalo, PA, US / Bridgeman Images

Comete Hale - Bopp - 03/1997 - Comet Hale - Bopp 03/1997 - Comete Hale - Bopp 12/03/1997 Batsto, NJ, USA. Comet Hale - Bopp on March 12, 1997 Batsto, NJ, USA
Comete Hale - Bopp - 03/1997 - Comet Hale - Bopp 03/1997 - Comete Hale - Bopp 12/03/1997 Batsto, NJ, USA. Comet Hale - Bopp on March 12, 1997 Batsto, NJ, USA

PIX4569618: Comete Hale - Bopp - 03/1997 - Comet Hale - Bopp 03/1997 - Comete Hale - Bopp 12/03/1997 Batsto, NJ, USA. Comet Hale - Bopp on March 12, 1997 Batsto, NJ, USA / Bridgeman Images

Comete Hale - Bopp and clusters open M34 - 04/1997 - Comet Hale - Bopp with open cluster M34 - This is the beautiful Comet Hale - Bopp as it as it passed by (from our point of view) the star cluster M34 in April of 1997. The solid portion or nucleus of the comet is made up of ice, frozen gases, dust and small rock. Compared to most comets Hale - Bopp is very large - about 35 kilometers in diameter. As its orbit brought it closer to the sun, the frozen mass began to melt and a coma, which is a gaseous cloud, developed around the nucleus. This coma has grown to be hundreds of thousands of miles in diameter. Finally the tail developed which became millions of miles long. (4 min. exposure on Kodak Pro 400 PPF film with 8 inch f/1.5 Schmidt camera
Comete Hale - Bopp and clusters open M34 - 04/1997 - Comet Hale - Bopp with open cluster M34 - This is the beautiful Comet Hale - Bopp as it as it passed by (from our point of view) the star cluster M34 in April of 1997. The solid portion or nucleus of the comet is made up of ice, frozen gases, dust and small rock. Compared to most comets Hale - Bopp is very large - about 35 kilometers in diameter. As its orbit brought it closer to the sun, the frozen mass began to melt and a coma, which is a gaseous cloud, developed around the nucleus. This coma has grown to be hundreds of thousands of miles in diameter. Finally the tail developed which became millions of miles long. (4 min. exposure on Kodak Pro 400 PPF film with 8 inch f/1.5 Schmidt camera

PIX4569806: Comete Hale - Bopp and clusters open M34 - 04/1997 - Comet Hale - Bopp with open cluster M34 - This is the beautiful Comet Hale - Bopp as it as it passed by (from our point of view) the star cluster M34 in April of 1997. The solid portion or nucleus of the comet is made up of ice, frozen gases, dust and small rock. Compared to most comets Hale - Bopp is very large - about 35 kilometers in diameter. As its orbit brought it closer to the sun, the frozen mass began to melt and a coma, which is a gaseous cloud, developed around the nucleus. This coma has grown to be hundreds of thousands of miles in diameter. Finally the tail developed which became millions of miles long. (4 min. exposure on Kodak Pro 400 PPF film with 8 inch f/1.5 Schmidt camera / Bridgeman Images

Observation of the eclipse of the Sun from 11/08/1999 - Solar eclipse observation - Observation of the sun with protective glasses. Fecamp. Solar eclipse observation with safe solar glasses. August 11 1999
Observation of the eclipse of the Sun from 11/08/1999 - Solar eclipse observation - Observation of the sun with protective glasses. Fecamp. Solar eclipse observation with safe solar glasses. August 11 1999

PIX4567295: Observation of the eclipse of the Sun from 11/08/1999 - Solar eclipse observation - Observation of the sun with protective glasses. Fecamp. Solar eclipse observation with safe solar glasses. August 11 1999 / Bridgeman Images

Eclipse of 11/08/1999: observation du soleil - Solar eclipse observation with safe solar glasses. August 11 1999 - Sun observation with protective glasses
Eclipse of 11/08/1999: observation du soleil - Solar eclipse observation with safe solar glasses. August 11 1999 - Sun observation with protective glasses

PIX4567325: Eclipse of 11/08/1999: observation du soleil - Solar eclipse observation with safe solar glasses. August 11 1999 - Sun observation with protective glasses / Bridgeman Images

Eclipse du 11/08/1999 - Solar eclipse of Aug 11 1999 - Observation of the sun with protective glasses. Total eclipse of Sun from 11/08/1999 in France. Solar eclipse observation with eclipse sunglasses. August 11 1999
Eclipse du 11/08/1999 - Solar eclipse of Aug 11 1999 - Observation of the sun with protective glasses. Total eclipse of Sun from 11/08/1999 in France. Solar eclipse observation with eclipse sunglasses. August 11 1999

PIX4567436: Eclipse du 11/08/1999 - Solar eclipse of Aug 11 1999 - Observation of the sun with protective glasses. Total eclipse of Sun from 11/08/1999 in France. Solar eclipse observation with eclipse sunglasses. August 11 1999 / Bridgeman Images

Open cluster NGC 6811 in Swan - Open cluster NGC 6811 in Cygnus - Star cluster NGC 6811 in the constellation Swan
Open cluster NGC 6811 in Swan - Open cluster NGC 6811 in Cygnus - Star cluster NGC 6811 in the constellation Swan

PIX4568487: Open cluster NGC 6811 in Swan - Open cluster NGC 6811 in Cygnus - Star cluster NGC 6811 in the constellation Swan / Bridgeman Images

Star cluster NGC 6791 in Lyra - Open cluster NGC 6791 in Lyra - NGC 6791 is one of the oldest and largest open clusters; it contains about 10,000 stars. Here, a detail of the cluster obtained by the Hubble space telescope. The stars present would be 8 billion years old. A galaxy in the background is also visible at the top left. NGC 6791 is one of the oldest and largest open clusters known, about 10 times larger than most open clusters and containing roughly 10,000 stars. The cluster is located 13 000 light years in the constellation Lyra. The full Hubble Advanced Camera for Surveys field is full of stars estimated to be 8 billion years old. Two background galaxies can be seen at upper left
Star cluster NGC 6791 in Lyra - Open cluster NGC 6791 in Lyra - NGC 6791 is one of the oldest and largest open clusters; it contains about 10,000 stars. Here, a detail of the cluster obtained by the Hubble space telescope. The stars present would be 8 billion years old. A galaxy in the background is also visible at the top left. NGC 6791 is one of the oldest and largest open clusters known, about 10 times larger than most open clusters and containing roughly 10,000 stars. The cluster is located 13 000 light years in the constellation Lyra. The full Hubble Advanced Camera for Surveys field is full of stars estimated to be 8 billion years old. Two background galaxies can be seen at upper left

PIX4568504: Star cluster NGC 6791 in Lyra - Open cluster NGC 6791 in Lyra - NGC 6791 is one of the oldest and largest open clusters; it contains about 10,000 stars. Here, a detail of the cluster obtained by the Hubble space telescope. The stars present would be 8 billion years old. A galaxy in the background is also visible at the top left. NGC 6791 is one of the oldest and largest open clusters known, about 10 times larger than most open clusters and containing roughly 10,000 stars. The cluster is located 13 000 light years in the constellation Lyra. The full Hubble Advanced Camera for Surveys field is full of stars estimated to be 8 billion years old. Two background galaxies can be seen at upper left / Bridgeman Images

Open cluster M29 in the Swan - Open cluster M29 in Cygnus - The cluster of stars M29 (NGC 6913) in the constellation Swan
Open cluster M29 in the Swan - Open cluster M29 in Cygnus - The cluster of stars M29 (NGC 6913) in the constellation Swan

PIX4568535: Open cluster M29 in the Swan - Open cluster M29 in Cygnus - The cluster of stars M29 (NGC 6913) in the constellation Swan / Bridgeman Images

Open cluster M52 in Cassiopee - Open cluster M52 in Cassiopei
Open cluster M52 in Cassiopee - Open cluster M52 in Cassiopei

PIX4568631: Open cluster M52 in Cassiopee - Open cluster M52 in Cassiopei / Bridgeman Images

Gallo Roman Art: mosaic paving representing a rustic calendar, Seeding and plowing scene, end 2nd, beginning of 3rd century AD (mosaic)
Gallo Roman Art: mosaic paving representing a rustic calendar, Seeding and plowing scene, end 2nd, beginning of 3rd century AD (mosaic)

JLJ4565043: Gallo Roman Art: mosaic paving representing a rustic calendar, Seeding and plowing scene, end 2nd, beginning of 3rd century AD (mosaic), Gallo-Roman, (2nd century AD) / Bridgeman Images

Globular cluster M56 in Lyre - Globular cluster M56 in Lyr
Globular cluster M56 in Lyre - Globular cluster M56 in Lyr

PIX4565048: Globular cluster M56 in Lyre - Globular cluster M56 in Lyr / Bridgeman Images

Gallo Roman Art: mosaic paving representing a rustic calendar, Scene of thatching, end 2nd, beginning of 3rd century AD (mosaic)
Gallo Roman Art: mosaic paving representing a rustic calendar, Scene of thatching, end 2nd, beginning of 3rd century AD (mosaic)

JLJ4565066: Gallo Roman Art: mosaic paving representing a rustic calendar, Scene of thatching, end 2nd, beginning of 3rd century AD (mosaic), Gallo-Roman, (2nd century AD) / Bridgeman Images

Globular cluster M71 in the Fleche - Globular cluster M71 in Sagitta - M71 (NGC 6838) is a globular cluster located in the constellation Fleche at a distance of about 12,000 years - light. M71 is a star cluster in the constellation Sagitta at about 12000 light - years from Earth. M71 is quite small, probably only 30 or so light - years across, although there are further outlying stars whose membership in M71 is uncertain
Globular cluster M71 in the Fleche - Globular cluster M71 in Sagitta - M71 (NGC 6838) is a globular cluster located in the constellation Fleche at a distance of about 12,000 years - light. M71 is a star cluster in the constellation Sagitta at about 12000 light - years from Earth. M71 is quite small, probably only 30 or so light - years across, although there are further outlying stars whose membership in M71 is uncertain

PIX4565077: Globular cluster M71 in the Fleche - Globular cluster M71 in Sagitta - M71 (NGC 6838) is a globular cluster located in the constellation Fleche at a distance of about 12,000 years - light. M71 is a star cluster in the constellation Sagitta at about 12000 light - years from Earth. M71 is quite small, probably only 30 or so light - years across, although there are further outlying stars whose membership in M71 is uncertain / Bridgeman Images

Central part of the Virgin galaxy cluster - Heart of the Virgo cluster of galaxies - The two elliptic galaxies are at the center M86 (NGC 4406), right M84 (NGC 4374). Image obtained with a 130 mm bezel. 1h pose M86 and M84 are two giant lenticular galaxies at the heart of the Virgo cluster of galaxies. NGC 4438, a spiral galaxy at the left of the photo, appears to be distorted by an interaction with nearby NGC 4435. Located about 70 million light years away, the Virgo cluster is a gigantic collection of several thousand galaxies that dominate our local part of the universe
Central part of the Virgin galaxy cluster - Heart of the Virgo cluster of galaxies - The two elliptic galaxies are at the center M86 (NGC 4406), right M84 (NGC 4374). Image obtained with a 130 mm bezel. 1h pose M86 and M84 are two giant lenticular galaxies at the heart of the Virgo cluster of galaxies. NGC 4438, a spiral galaxy at the left of the photo, appears to be distorted by an interaction with nearby NGC 4435. Located about 70 million light years away, the Virgo cluster is a gigantic collection of several thousand galaxies that dominate our local part of the universe

PIX4565399: Central part of the Virgin galaxy cluster - Heart of the Virgo cluster of galaxies - The two elliptic galaxies are at the center M86 (NGC 4406), right M84 (NGC 4374). Image obtained with a 130 mm bezel. 1h pose M86 and M84 are two giant lenticular galaxies at the heart of the Virgo cluster of galaxies. NGC 4438, a spiral galaxy at the left of the photo, appears to be distorted by an interaction with nearby NGC 4435. Located about 70 million light years away, the Virgo cluster is a gigantic collection of several thousand galaxies that dominate our local part of the universe / Bridgeman Images

The Virgo cluster of galaxies - The Virgo cluster of galaxies - The Virgin cluster contains about 2000 galaxies. In the middle of the picture, the giant elliptical galaxy M87. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. Image of the central portion of the great Virgo/Coma cluster including Markarians chain. Located about 70 million light years away, The Virgo cluster is a gigantic collection of several thousand galaxies that dominate our local part of the universe. Image taken with the Palomar Observatory 48 - inch Schmidt telescope as part of the Digitized Sky Survey
The Virgo cluster of galaxies - The Virgo cluster of galaxies - The Virgin cluster contains about 2000 galaxies. In the middle of the picture, the giant elliptical galaxy M87. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. Image of the central portion of the great Virgo/Coma cluster including Markarians chain. Located about 70 million light years away, The Virgo cluster is a gigantic collection of several thousand galaxies that dominate our local part of the universe. Image taken with the Palomar Observatory 48 - inch Schmidt telescope as part of the Digitized Sky Survey

PIX4565507: The Virgo cluster of galaxies - The Virgo cluster of galaxies - The Virgin cluster contains about 2000 galaxies. In the middle of the picture, the giant elliptical galaxy M87. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. Image of the central portion of the great Virgo/Coma cluster including Markarians chain. Located about 70 million light years away, The Virgo cluster is a gigantic collection of several thousand galaxies that dominate our local part of the universe. Image taken with the Palomar Observatory 48 - inch Schmidt telescope as part of the Digitized Sky Survey / Bridgeman Images

Galaxy Cluster Abell S0740 in Centaurus - Galaxy Cluster Abell S0740 in Centaurus - The Hubble space telescope photographed a cluster of galaxies 450 million years ago - Earth light, Abell S0740. There are galaxies of various shapes alongside the giant elliptical galaxy ESO 325 - G004. Image obtained by the ACS camera in January 2005 and February 2006. Hubble Space Telescope image showing the diverse collection of galaxies in a galaxy cluster Abell S0740, at about 450 million light - years away in the constellation Centaurus. The giant elliptical galaxy ESO 325 - G004 looms large at the club's center
Galaxy Cluster Abell S0740 in Centaurus - Galaxy Cluster Abell S0740 in Centaurus - The Hubble space telescope photographed a cluster of galaxies 450 million years ago - Earth light, Abell S0740. There are galaxies of various shapes alongside the giant elliptical galaxy ESO 325 - G004. Image obtained by the ACS camera in January 2005 and February 2006. Hubble Space Telescope image showing the diverse collection of galaxies in a galaxy cluster Abell S0740, at about 450 million light - years away in the constellation Centaurus. The giant elliptical galaxy ESO 325 - G004 looms large at the club's center

PIX4565560: Galaxy Cluster Abell S0740 in Centaurus - Galaxy Cluster Abell S0740 in Centaurus - The Hubble space telescope photographed a cluster of galaxies 450 million years ago - Earth light, Abell S0740. There are galaxies of various shapes alongside the giant elliptical galaxy ESO 325 - G004. Image obtained by the ACS camera in January 2005 and February 2006. Hubble Space Telescope image showing the diverse collection of galaxies in a galaxy cluster Abell S0740, at about 450 million light - years away in the constellation Centaurus. The giant elliptical galaxy ESO 325 - G004 looms large at the club's center / Bridgeman Images

Gallo Roman Art: mosaic paving representing a rustic calendar, Sowing feves, end 2nd, beginning of 3rd century AD (mosaic)
Gallo Roman Art: mosaic paving representing a rustic calendar, Sowing feves, end 2nd, beginning of 3rd century AD (mosaic)

JLJ4565062: Gallo Roman Art: mosaic paving representing a rustic calendar, Sowing feves, end 2nd, beginning of 3rd century AD (mosaic), Gallo-Roman, (2nd century AD) / Bridgeman Images

The social housing of Fernand Pouillon (1912-1986), completed in 1950, in Meudon la Foret (Hauts de Seine).
The social housing of Fernand Pouillon (1912-1986), completed in 1950, in Meudon la Foret (Hauts de Seine).

TEC4565159: The social housing of Fernand Pouillon (1912-1986), completed in 1950, in Meudon la Foret (Hauts de Seine)., Pouillon, Fernand (1912-86) / Bridgeman Images

Coma cluster of galaxies Abell 1656 - Coma cluster of galaxies - The Comas cluster is a large cluster of galaxies, comprising several thousand galaxies. It is located more than 300 million light years ago in the constellation Coma Berenices (Berenice Hair). This photo from the Hubble Space Telescope shows part of the cluster of a brilliant spiral galaxy, IC 4040, in the top left, and many elliptical galaxies. Also known as Abell 1656, the Coma Cluster is over 300 million light - years away. The cluster, named after its parent constellation Coma Berenices, is near the Milky Way's north pole. This places the Coma Cluster in an area unobscured by dust and gas from the plane of the Milky Way, and easily visible by Earth viewers. This Hubble image consists of a section of the cluster that is roughly one - third of the way out from the center of the cluster. One bright spiral galaxy is visible in the upper left of the image. It is distinctly brighter and bluer than galaxies surrounding it. A series of dusty spiral arms appears reddish brown against the whiter disk of the galaxy, and gives rise to the idea that this galaxy has been disturbed at some point in the past. The other galaxies in the image are either elliptical, S0 galaxies, or background galaxies far beyond the Coma Cluster sphere
Coma cluster of galaxies Abell 1656 - Coma cluster of galaxies - The Comas cluster is a large cluster of galaxies, comprising several thousand galaxies. It is located more than 300 million light years ago in the constellation Coma Berenices (Berenice Hair). This photo from the Hubble Space Telescope shows part of the cluster of a brilliant spiral galaxy, IC 4040, in the top left, and many elliptical galaxies. Also known as Abell 1656, the Coma Cluster is over 300 million light - years away. The cluster, named after its parent constellation Coma Berenices, is near the Milky Way's north pole. This places the Coma Cluster in an area unobscured by dust and gas from the plane of the Milky Way, and easily visible by Earth viewers. This Hubble image consists of a section of the cluster that is roughly one - third of the way out from the center of the cluster. One bright spiral galaxy is visible in the upper left of the image. It is distinctly brighter and bluer than galaxies surrounding it. A series of dusty spiral arms appears reddish brown against the whiter disk of the galaxy, and gives rise to the idea that this galaxy has been disturbed at some point in the past. The other galaxies in the image are either elliptical, S0 galaxies, or background galaxies far beyond the Coma Cluster sphere

PIX4565294: Coma cluster of galaxies Abell 1656 - Coma cluster of galaxies - The Comas cluster is a large cluster of galaxies, comprising several thousand galaxies. It is located more than 300 million light years ago in the constellation Coma Berenices (Berenice Hair). This photo from the Hubble Space Telescope shows part of the cluster of a brilliant spiral galaxy, IC 4040, in the top left, and many elliptical galaxies. Also known as Abell 1656, the Coma Cluster is over 300 million light - years away. The cluster, named after its parent constellation Coma Berenices, is near the Milky Way's north pole. This places the Coma Cluster in an area unobscured by dust and gas from the plane of the Milky Way, and easily visible by Earth viewers. This Hubble image consists of a section of the cluster that is roughly one - third of the way out from the center of the cluster. One bright spiral galaxy is visible in the upper left of the image. It is distinctly brighter and bluer than galaxies surrounding it. A series of dusty spiral arms appears reddish brown against the whiter disk of the galaxy, and gives rise to the idea that this galaxy has been disturbed at some point in the past. The other galaxies in the image are either elliptical, S0 galaxies, or background galaxies far beyond the Coma Cluster sphere / Bridgeman Images

The social housing of Fernand Pouillon (1912-1986), completed in 1950, in Meudon la Foret (Hauts de Seine).
The social housing of Fernand Pouillon (1912-1986), completed in 1950, in Meudon la Foret (Hauts de Seine).

TEC4565389: The social housing of Fernand Pouillon (1912-1986), completed in 1950, in Meudon la Foret (Hauts de Seine)., Pouillon, Fernand (1912-86) / Bridgeman Images

Central part of the Virgo cluster of galaxies - Central part of the Virgo cluster of galaxies - On the right the M84 (NGC 4374) and M86 (NGC 4406) (to its left) dominate the image. Lower left is the elliptical galaxy M87. The nearest moderately rich cluster of galaxies lies in the direction of Virgo. The richest part of the cluster is centred on the giant elliptical - lenticular galaxies M84 (NGC 4374) (right) and M86 (NGC 4406) (left) which dominate this picture. However, the dynamical centre of the cluster is M87, to the lower left (south east) of this picture
Central part of the Virgo cluster of galaxies - Central part of the Virgo cluster of galaxies - On the right the M84 (NGC 4374) and M86 (NGC 4406) (to its left) dominate the image. Lower left is the elliptical galaxy M87. The nearest moderately rich cluster of galaxies lies in the direction of Virgo. The richest part of the cluster is centred on the giant elliptical - lenticular galaxies M84 (NGC 4374) (right) and M86 (NGC 4406) (left) which dominate this picture. However, the dynamical centre of the cluster is M87, to the lower left (south east) of this picture

PIX4565403: Central part of the Virgo cluster of galaxies - Central part of the Virgo cluster of galaxies - On the right the M84 (NGC 4374) and M86 (NGC 4406) (to its left) dominate the image. Lower left is the elliptical galaxy M87. The nearest moderately rich cluster of galaxies lies in the direction of Virgo. The richest part of the cluster is centred on the giant elliptical - lenticular galaxies M84 (NGC 4374) (right) and M86 (NGC 4406) (left) which dominate this picture. However, the dynamical centre of the cluster is M87, to the lower left (south east) of this picture / Bridgeman Images

Le mur des Names au Memorial de la Shoah, 17 rue Geoffroy l'Asnier, Paris 4. Architect Antoine Jouve, Simon Vignaud, 2005
Le mur des Names au Memorial de la Shoah, 17 rue Geoffroy l'Asnier, Paris 4. Architect Antoine Jouve, Simon Vignaud, 2005

LBY4553088: Le mur des Names au Memorial de la Shoah, 17 rue Geoffroy l'Asnier, Paris 4. Architect Antoine Jouve, Simon Vignaud, 2005 / Bridgeman Images

In the heart of the Renault trapeze, the headquarters of the pharmaceutical laboratory “Beaufour Ipsen Pharma”, Khapa, 65 Quai Georges Gorse to Boulogne Billancourt (Boulogne-Billancourt), Hauts-de-Seine (Hauts de Seine), Ile de France (Ile-de-France), France. Architecture by Norman Forster, 2008
In the heart of the Renault trapeze, the headquarters of the pharmaceutical laboratory “Beaufour Ipsen Pharma”, Khapa, 65 Quai Georges Gorse to Boulogne Billancourt (Boulogne-Billancourt), Hauts-de-Seine (Hauts de Seine), Ile de France (Ile-de-France), France. Architecture by Norman Forster, 2008

LBY4552411: In the heart of the Renault trapeze, the headquarters of the pharmaceutical laboratory “Beaufour Ipsen Pharma”, Khapa, 65 Quai Georges Gorse to Boulogne Billancourt (Boulogne-Billancourt), Hauts-de-Seine (Hauts de Seine), Ile de France (Ile-de-France), France. Architecture by Norman Forster, 2008, Foster, Norman (b.1935) / Bridgeman Images

The extension of the “Meteo France Ouest” Centre, 27 rue Jules Valles, Saint Jacques de la Lande, Ille et Vilaine (Ille et Vilaine), Brittany. Architecture by Yves-Marie Maurer, 2009. Photography 1/9/2009.
The extension of the “Meteo France Ouest” Centre, 27 rue Jules Valles, Saint Jacques de la Lande, Ille et Vilaine (Ille et Vilaine), Brittany. Architecture by Yves-Marie Maurer, 2009. Photography 1/9/2009.

MDA4552417: The extension of the “Meteo France Ouest” Centre, 27 rue Jules Valles, Saint Jacques de la Lande, Ille et Vilaine (Ille et Vilaine), Brittany. Architecture by Yves-Marie Maurer, 2009. Photography 1/9/2009., Maurer, Yves-Marie (21st century) / Bridgeman Images

The extension of the “Meteo France Ouest” Centre, 27 rue Jules Valles, Saint Jacques de la Lande, Ille et Vilaine (Ille et Vilaine), Brittany. Architecture by Yves-Marie Maurer, 2009. Photography 1/9/2009.
The extension of the “Meteo France Ouest” Centre, 27 rue Jules Valles, Saint Jacques de la Lande, Ille et Vilaine (Ille et Vilaine), Brittany. Architecture by Yves-Marie Maurer, 2009. Photography 1/9/2009.

MDA4552435: The extension of the “Meteo France Ouest” Centre, 27 rue Jules Valles, Saint Jacques de la Lande, Ille et Vilaine (Ille et Vilaine), Brittany. Architecture by Yves-Marie Maurer, 2009. Photography 1/9/2009., Maurer, Yves-Marie (21st century) / Bridgeman Images

Figures of musical angels, sculpted on the south wall of the choir of the Cathedrale Notre-Dame de Paris built at the beginning of the 14th century Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc -
Figures of musical angels, sculpted on the south wall of the choir of the Cathedrale Notre-Dame de Paris built at the beginning of the 14th century Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc -

ITR4553697: Figures of musical angels, sculpted on the south wall of the choir of the Cathedrale Notre-Dame de Paris built at the beginning of the 14th century Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc - / Bridgeman Images

The extension of the “Meteo France Ouest” Centre, 27 rue Jules Valles, Saint Jacques de la Lande, Ille et Vilaine (Ille et Vilaine), Brittany. Architecture by Yves-Marie Maurer, 2009. Photography 1/9/2009.
The extension of the “Meteo France Ouest” Centre, 27 rue Jules Valles, Saint Jacques de la Lande, Ille et Vilaine (Ille et Vilaine), Brittany. Architecture by Yves-Marie Maurer, 2009. Photography 1/9/2009.

MDA4552449: The extension of the “Meteo France Ouest” Centre, 27 rue Jules Valles, Saint Jacques de la Lande, Ille et Vilaine (Ille et Vilaine), Brittany. Architecture by Yves-Marie Maurer, 2009. Photography 1/9/2009., Maurer, Yves-Marie (21st century) / Bridgeman Images

Hotel industrielle, Paris 15 (Industrial hotel in Paris). Architecture by Paul Chemetov and Borja Huidobro, 1992.
Hotel industrielle, Paris 15 (Industrial hotel in Paris). Architecture by Paul Chemetov and Borja Huidobro, 1992.

TEC4552567: Hotel industrielle, Paris 15 (Industrial hotel in Paris). Architecture by Paul Chemetov and Borja Huidobro, 1992., Huidobro, Borja (b.1936) Chemetov, Paul (b.1928) / Bridgeman Images

The headquarters of Canal+(Canal+headquarters), Paris 15. Architecture by Richard Meier, 1992.
The headquarters of Canal+(Canal+headquarters), Paris 15. Architecture by Richard Meier, 1992.

TEC4552601: The headquarters of Canal+(Canal+headquarters), Paris 15. Architecture by Richard Meier, 1992., Meier, Richard (b.1934) / Bridgeman Images

Cathedrale de la Resurrection, 12 courses Monseigneur Romero, Evry (Essonne, France). Architect Mario Botta, 1995.
Cathedrale de la Resurrection, 12 courses Monseigneur Romero, Evry (Essonne, France). Architect Mario Botta, 1995.

TEC4552734: Cathedrale de la Resurrection, 12 courses Monseigneur Romero, Evry (Essonne, France). Architect Mario Botta, 1995., Botta, Mario (b.1943) / Bridgeman Images


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