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Lovejoy Comet - December 2011 - Comet Lovejoy - December 2011 - Lovejoy Comet seen in Chile on December 23, 2011. Comet Lovejoy seen from Chile on Dec. 23, 2011
Lovejoy Comet - December 2011 - Comet Lovejoy - December 2011 - Lovejoy Comet seen in Chile on December 23, 2011. Comet Lovejoy seen from Chile on Dec. 23, 2011

PIX4571198: Lovejoy Comet - December 2011 - Comet Lovejoy - December 2011 - Lovejoy Comet seen in Chile on December 23, 2011. Comet Lovejoy seen from Chile on Dec. 23, 2011 / Bridgeman Images

ID: PIX4571198

Lovejoy Comet - December 2011 - Comet Lovejoy - December 2011 - Lovejoy Comet seen in Chile on December 23, 2011. Comet Lovejoy seen from Chile on Dec. 23, 2011

Lovejoy Comet - December 2011 - Lovejoy Comet seen in Australia, (Yorkrakine Rock). 26 December 2011. Comet Lovejoy wide - angle taken near Yorkrakine Rock, West Australia on Dec. 26, 201
Lovejoy Comet - December 2011 - Lovejoy Comet seen in Australia, (Yorkrakine Rock). 26 December 2011. Comet Lovejoy wide - angle taken near Yorkrakine Rock, West Australia on Dec. 26, 201

PIX4571217: Lovejoy Comet - December 2011 - Lovejoy Comet seen in Australia, (Yorkrakine Rock). 26 December 2011. Comet Lovejoy wide - angle taken near Yorkrakine Rock, West Australia on Dec. 26, 201 / Bridgeman Images

ID: PIX4571217

Lovejoy Comet - December 2011 - Lovejoy Comet seen in Australia, (Yorkrakine Rock). 26 December 2011. Comet Lovejoy wide - angle taken near Yorkrakine Rock, West Australia on Dec. 26, 201

Galerie Vivienne in Paris 2nd arrondissement. Construction 1823-1826, architect Jacques Delannoy.
Galerie Vivienne in Paris 2nd arrondissement. Construction 1823-1826, architect Jacques Delannoy.

TEC4571245: Galerie Vivienne in Paris 2nd arrondissement. Construction 1823-1826, architect Jacques Delannoy. / Bridgeman Images

ID: TEC4571245

Galerie Vivienne in Paris 2nd arrondissement. Construction 1823-1826, architect Jacques Delannoy.

The ISON Comete - 05/2013 - The ISON Comet seen on May 8, 2013 by the Hubble Space Telescope (HST). Hubble Space Telescope image showing comet ISON on May 8 2013
The ISON Comete - 05/2013 - The ISON Comet seen on May 8, 2013 by the Hubble Space Telescope (HST). Hubble Space Telescope image showing comet ISON on May 8 2013

PIX4571310: The ISON Comete - 05/2013 - The ISON Comet seen on May 8, 2013 by the Hubble Space Telescope (HST). Hubble Space Telescope image showing comet ISON on May 8 2013 / Bridgeman Images

ID: PIX4571310

The ISON Comete - 05/2013 - The ISON Comet seen on May 8, 2013 by the Hubble Space Telescope (HST). Hubble Space Telescope image showing comet ISON on May 8 2013

Boulevard de Saint Denis and Boulevard Bonne Nouvelle in Paris 2nd arrondissement.
Boulevard de Saint Denis and Boulevard Bonne Nouvelle in Paris 2nd arrondissement.

TEC4571356: Boulevard de Saint Denis and Boulevard Bonne Nouvelle in Paris 2nd arrondissement. / Bridgeman Images

ID: TEC4571356

Boulevard de Saint Denis and Boulevard Bonne Nouvelle in Paris 2nd arrondissement.

La Bibliotheque de France, Richelieu site in Paris 2nd arrondissement. Construction 1869, architect Henri Labrouste (1801-1875).
La Bibliotheque de France, Richelieu site in Paris 2nd arrondissement. Construction 1869, architect Henri Labrouste (1801-1875).

TEC4571370: La Bibliotheque de France, Richelieu site in Paris 2nd arrondissement. Construction 1869, architect Henri Labrouste (1801-1875). / Bridgeman Images

ID: TEC4571370

La Bibliotheque de France, Richelieu site in Paris 2nd arrondissement. Construction 1869, architect Henri Labrouste (1801-1875).

Rue Saint Sauveur in Paris 2nd arrondissement.
Rue Saint Sauveur in Paris 2nd arrondissement.

TEC4571378: Rue Saint Sauveur in Paris 2nd arrondissement. / Bridgeman Images

ID: TEC4571378

Rue Saint Sauveur in Paris 2nd arrondissement.

Rue de Montorgueil in Paris.
Rue de Montorgueil in Paris.

TEC4571561: Rue de Montorgueil in Paris. / Bridgeman Images

ID: TEC4571561

Rue de Montorgueil in Paris.

Summer Triangle - Summer Triangle - The Summer Triangle is an asterism formed by the brilliant stars Deneb (at the top of the picture, in the Swan), Vega (on the right in the Lyre) and Altair (on the left, in the Eagle). Summer Triangle is an asterism made of three bright stars: Deneb (top in Cygnus, Vega (right in Lyra) and Altair (left in Aquila)
Summer Triangle - Summer Triangle - The Summer Triangle is an asterism formed by the brilliant stars Deneb (at the top of the picture, in the Swan), Vega (on the right in the Lyre) and Altair (on the left, in the Eagle). Summer Triangle is an asterism made of three bright stars: Deneb (top in Cygnus, Vega (right in Lyra) and Altair (left in Aquila)

PIX4571607: Summer Triangle - Summer Triangle - The Summer Triangle is an asterism formed by the brilliant stars Deneb (at the top of the picture, in the Swan), Vega (on the right in the Lyre) and Altair (on the left, in the Eagle). Summer Triangle is an asterism made of three bright stars: Deneb (top in Cygnus, Vega (right in Lyra) and Altair (left in Aquila) / Bridgeman Images

ID: PIX4571607

Summer Triangle - Summer Triangle - The Summer Triangle is an asterism formed by the brilliant stars Deneb (at the top of the picture, in the Swan), Vega (on the right in the Lyre) and Altair (on the left, in the Eagle). Summer Triangle is an asterism made of three bright stars: Deneb (top in Cygnus, Vega (right in Lyra) and Altair (left in Aquila)

Constellation of the Great Bear - Constellation of Ursa Major: Plate extracted from the Mirror of Urania -1824. Ursa Major, the constellation of the Great Bear, from Urania's Mirror, a colourful set of constellation cards published in 1824. Over the years, the star at the end of the tail has been known by two popular names, Alkaid and Benetnasch but Alkaid is now the official name
Constellation of the Great Bear - Constellation of Ursa Major: Plate extracted from the Mirror of Urania -1824. Ursa Major, the constellation of the Great Bear, from Urania's Mirror, a colourful set of constellation cards published in 1824. Over the years, the star at the end of the tail has been known by two popular names, Alkaid and Benetnasch but Alkaid is now the official name

PIX4571623: Constellation of the Great Bear - Constellation of Ursa Major: Plate extracted from the Mirror of Urania -1824. Ursa Major, the constellation of the Great Bear, from Urania's Mirror, a colourful set of constellation cards published in 1824. Over the years, the star at the end of the tail has been known by two popular names, Alkaid and Benetnasch but Alkaid is now the official name / Bridgeman Images

ID: PIX4571623

Constellation of the Great Bear - Constellation of Ursa Major: Plate extracted from the Mirror of Urania -1824. Ursa Major, the constellation of the Great Bear, from Urania's Mirror, a colourful set of constellation cards published in 1824. Over the years, the star at the end of the tail has been known by two popular names, Alkaid and Benetnasch but Alkaid is now the official name

Rue de Montorgueil in Paris.
Rue de Montorgueil in Paris.

TEC4571631: Rue de Montorgueil in Paris. / Bridgeman Images

ID: TEC4571631

Rue de Montorgueil in Paris.

Building 226 rue Saint Denis in Paris.
Building 226 rue Saint Denis in Paris.

TEC4571637: Building 226 rue Saint Denis in Paris. / Bridgeman Images

ID: TEC4571637

Building 226 rue Saint Denis in Paris.

Rue de Montorgueil in Paris.
Rue de Montorgueil in Paris.

TEC4571660: Rue de Montorgueil in Paris. / Bridgeman Images

ID: TEC4571660

Rue de Montorgueil in Paris.

La Maison Doree, 20 boulevard des Italians in Paris. 1835 construction, architect Victor Lemaire.
La Maison Doree, 20 boulevard des Italians in Paris. 1835 construction, architect Victor Lemaire.

TEC4571727: La Maison Doree, 20 boulevard des Italians in Paris. 1835 construction, architect Victor Lemaire. / Bridgeman Images

ID: TEC4571727

La Maison Doree, 20 boulevard des Italians in Paris. 1835 construction, architect Victor Lemaire.

Star Vega in the Lyre - Star Vega in infrared - Vega (Alpha Lyrae) is the main star of the constellation Lyra, located only 25.4 light years from the Sun. It is the second brightest star after Sirius in the northern hemisphere. It's seen here in infrared by the Spitzer space telescope. Observed in this wavelength, the dust cloud surrounding the star appears. Nasa's Spitzer Space Telescope captured these images of the star Vega, located 25 light years away in the constellation Lyra. Spitzer was able to detect the heat radiation from the cloud of dust around the star and found that the debris disk is much larger than previously thought. This side - by - side comparison, taken by Spitzer's multiband imaging photometer, shows the warm infrared glows from dust particles orbiting the star at wavelengths of 24 microns (on the left in blue) and 70 microns (on the right in red). Both images show a very large, circular and smooth debris disk. The disk radius extends to at least 815 astronomical units. (One astronomical unit is the distance from Earth to the Sun, which is 150 - million kilometers or 93 - million miles). Scientists compared the surface brightness of the disk in the infrared wavelengths to determine the temperature distribution of the disk and then refer the corresponding particle size in the disk. Most of the particles in the disk are only a few microns in size, or 100 times smaller than a grain of Earth sand. These fine dust particles originate from collisions of embryonic planets near the star at a radius of approximately 90 astronomical units, and are then blown away by Vega's intense radiation. The mass and short lifetime of these small particles indicate that the disk detected by Spitzer is the aftermath of a large and relatively recent collision, involving bodies perhaps as big as the planet Pluto. The images are 3 arcminutes on each side. North is oriented upward and east is to the left
Star Vega in the Lyre - Star Vega in infrared - Vega (Alpha Lyrae) is the main star of the constellation Lyra, located only 25.4 light years from the Sun. It is the second brightest star after Sirius in the northern hemisphere. It's seen here in infrared by the Spitzer space telescope. Observed in this wavelength, the dust cloud surrounding the star appears. Nasa's Spitzer Space Telescope captured these images of the star Vega, located 25 light years away in the constellation Lyra. Spitzer was able to detect the heat radiation from the cloud of dust around the star and found that the debris disk is much larger than previously thought. This side - by - side comparison, taken by Spitzer's multiband imaging photometer, shows the warm infrared glows from dust particles orbiting the star at wavelengths of 24 microns (on the left in blue) and 70 microns (on the right in red). Both images show a very large, circular and smooth debris disk. The disk radius extends to at least 815 astronomical units. (One astronomical unit is the distance from Earth to the Sun, which is 150 - million kilometers or 93 - million miles). Scientists compared the surface brightness of the disk in the infrared wavelengths to determine the temperature distribution of the disk and then refer the corresponding particle size in the disk. Most of the particles in the disk are only a few microns in size, or 100 times smaller than a grain of Earth sand. These fine dust particles originate from collisions of embryonic planets near the star at a radius of approximately 90 astronomical units, and are then blown away by Vega's intense radiation. The mass and short lifetime of these small particles indicate that the disk detected by Spitzer is the aftermath of a large and relatively recent collision, involving bodies perhaps as big as the planet Pluto. The images are 3 arcminutes on each side. North is oriented upward and east is to the left

PIX4571758: Star Vega in the Lyre - Star Vega in infrared - Vega (Alpha Lyrae) is the main star of the constellation Lyra, located only 25.4 light years from the Sun. It is the second brightest star after Sirius in the northern hemisphere. It's seen here in infrared by the Spitzer space telescope. Observed in this wavelength, the dust cloud surrounding the star appears. Nasa's Spitzer Space Telescope captured these images of the star Vega, located 25 light years away in the constellation Lyra. Spitzer was able to detect the heat radiation from the cloud of dust around the star and found that the debris disk is much larger than previously thought. This side - by - side comparison, taken by Spitzer's multiband imaging photometer, shows the warm infrared glows from dust particles orbiting the star at wavelengths of 24 microns (on the left in blue) and 70 microns (on the right in red). Both images show a very large, circular and smooth debris disk. The disk radius extends to at least 815 astronomical units. (One astronomical unit is the distance from Earth to the Sun, which is 150 - million kilometers or 93 - million miles). Scientists compared the surface brightness of the disk in the infrared wavelengths to determine the temperature distribution of the disk and then refer the corresponding particle size in the disk. Most of the particles in the disk are only a few microns in size, or 100 times smaller than a grain of Earth sand. These fine dust particles originate from collisions of embryonic planets near the star at a radius of approximately 90 astronomical units, and are then blown away by Vega's intense radiation. The mass and short lifetime of these small particles indicate that the disk detected by Spitzer is the aftermath of a large and relatively recent collision, involving bodies perhaps as big as the planet Pluto. The images are 3 arcminutes on each side. North is oriented upward and east is to the left / Bridgeman Images

ID: PIX4571758

Star Vega in the Lyre - Star Vega in infrared - Vega (Alpha Lyrae) is the main star of the constellation Lyra, located only 25.4 light years from the Sun. It is the second brightest star after Sirius in the northern hemisphere. It's seen here in infrared by the Spitzer space telescope. Observed in this wavelength, the dust cloud surrounding the star appears. Nasa's Spitzer Space Telescope captured these images of the star Vega, located 25 light years away in the constellation Lyra. Spitzer was able to detect the heat radiation from the cloud of dust around the star and found that the debris disk is much larger than previously thought. This side - by - side comparison, taken by Spitzer's multiband imaging photometer, shows the warm infrared glows from dust particles orbiting the star at wavelengths of 24 microns (on the left in blue) and 70 microns (on the right in red). Both images show a very large, circular and smooth debris disk. The disk radius extends to at least 815 astronomical

Proxima Star of Centauri - Proxima Centauri - Proxima of Centaur (in the center of the image) is the closest star to the Sun, at a distance of 4.2 years - light. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. Proxima Centauri is the nearest known star to the sun, at a distance of about 4.2 light years. It is an intrinsically faint red star, more than ten magnitudes (ten thousand times) fainter than the Sun. It is also much cooler, with a surface temperature of about 3100 C. Its visual (apparent) magnitude is eleven, so it is only visible with a good telescope, and only then from southern latitudes. Proxima is about one - tenth the mass of the sun, which accounts for its low surface temperature. It is possibly an outlying member of the triple alpha Centauri system just a few light days closer to us than the other, much brighter stars in the group
Proxima Star of Centauri - Proxima Centauri - Proxima of Centaur (in the center of the image) is the closest star to the Sun, at a distance of 4.2 years - light. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. Proxima Centauri is the nearest known star to the sun, at a distance of about 4.2 light years. It is an intrinsically faint red star, more than ten magnitudes (ten thousand times) fainter than the Sun. It is also much cooler, with a surface temperature of about 3100 C. Its visual (apparent) magnitude is eleven, so it is only visible with a good telescope, and only then from southern latitudes. Proxima is about one - tenth the mass of the sun, which accounts for its low surface temperature. It is possibly an outlying member of the triple alpha Centauri system just a few light days closer to us than the other, much brighter stars in the group

PIX4571821: Proxima Star of Centauri - Proxima Centauri - Proxima of Centaur (in the center of the image) is the closest star to the Sun, at a distance of 4.2 years - light. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. Proxima Centauri is the nearest known star to the sun, at a distance of about 4.2 light years. It is an intrinsically faint red star, more than ten magnitudes (ten thousand times) fainter than the Sun. It is also much cooler, with a surface temperature of about 3100 C. Its visual (apparent) magnitude is eleven, so it is only visible with a good telescope, and only then from southern latitudes. Proxima is about one - tenth the mass of the sun, which accounts for its low surface temperature. It is possibly an outlying member of the triple alpha Centauri system just a few light days closer to us than the other, much brighter stars in the group / Bridgeman Images

ID: PIX4571821

Proxima Star of Centauri - Proxima Centauri - Proxima of Centaur (in the center of the image) is the closest star to the Sun, at a distance of 4.2 years - light. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. Proxima Centauri is the nearest known star to the sun, at a distance of about 4.2 light years. It is an intrinsically faint red star, more than ten magnitudes (ten thousand times) fainter than the Sun. It is also much cooler, with a surface temperature of about 3100 C. Its visual (apparent) magnitude is eleven, so it is only visible with a good telescope, and only then from southern latitudes. Proxima is about one - tenth the mass of the sun, which accounts for its low surface temperature. It is possibly an outlying member of the triple alpha Centauri system just a few light days closer to us than the other, much brighter stars in the group

Le Peer Trianon a Versailles, architect Jacques Anges Gabriel, 1760-1764. Parc du Chateau de Versailles (Yvelines, Ile de France).
Le Peer Trianon a Versailles, architect Jacques Anges Gabriel, 1760-1764. Parc du Chateau de Versailles (Yvelines, Ile de France).

TEC4561685: Le Peer Trianon a Versailles, architect Jacques Anges Gabriel, 1760-1764. Parc du Chateau de Versailles (Yvelines, Ile de France). / Bridgeman Images

ID: TEC4561685

Le Peer Trianon a Versailles, architect Jacques Anges Gabriel, 1760-1764. Parc du Chateau de Versailles (Yvelines, Ile de France).

Vault with Corinthian columns of LaChapelle royale began by Jules Hardouin Mansart (1646-1708) in 1699 and completed in 1710 by Robert De Cotte (1656-1735).Chateau de Versailles (Les Yvelines). Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708), 1660-1700.
Vault with Corinthian columns of LaChapelle royale began by Jules Hardouin Mansart (1646-1708) in 1699 and completed in 1710 by Robert De Cotte (1656-1735).Chateau de Versailles (Les Yvelines). Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708), 1660-1700.

ITR4561887: Vault with Corinthian columns of LaChapelle royale began by Jules Hardouin Mansart (1646-1708) in 1699 and completed in 1710 by Robert De Cotte (1656-1735).Chateau de Versailles (Les Yvelines). Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708), 1660-1700. / Bridgeman Images

ID: ITR4561887

Vault with Corinthian columns of LaChapelle royale began by Jules Hardouin Mansart (1646-1708) in 1699 and completed in 1710 by Robert De Cotte (1656-1735).Chateau de Versailles (Les Yvelines). Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708), 1660-1700.

Saint-Louis Church, Versailles (Les Yvelines). Architect Jacques Hardouin Mansart De Sagonne (1709-1776), 1743-1754.
Saint-Louis Church, Versailles (Les Yvelines). Architect Jacques Hardouin Mansart De Sagonne (1709-1776), 1743-1754.

ITR4561932: Saint-Louis Church, Versailles (Les Yvelines). Architect Jacques Hardouin Mansart De Sagonne (1709-1776), 1743-1754. / Bridgeman Images

ID: ITR4561932

Saint-Louis Church, Versailles (Les Yvelines). Architect Jacques Hardouin Mansart De Sagonne (1709-1776), 1743-1754.

The dairy in the hamlet of the Queen in the northwest part of the garden of the Peer Trianon, built in 1782 by Hubert Robert (1733-1808). Chateau de Versailles (Les Yvelines), 1660-1700. Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708).
The dairy in the hamlet of the Queen in the northwest part of the garden of the Peer Trianon, built in 1782 by Hubert Robert (1733-1808). Chateau de Versailles (Les Yvelines), 1660-1700. Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708).

ITR4561943: The dairy in the hamlet of the Queen in the northwest part of the garden of the Peer Trianon, built in 1782 by Hubert Robert (1733-1808). Chateau de Versailles (Les Yvelines), 1660-1700. Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708). / Bridgeman Images

ID: ITR4561943

The dairy in the hamlet of the Queen in the northwest part of the garden of the Peer Trianon, built in 1782 by Hubert Robert (1733-1808). Chateau de Versailles (Les Yvelines), 1660-1700. Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708).

La Colonnade in the Parc du Chateau de Versailles (Les Yvelines), 1660-1700. Gardens of Andre Le Notre (1613-1700) and principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708).
La Colonnade in the Parc du Chateau de Versailles (Les Yvelines), 1660-1700. Gardens of Andre Le Notre (1613-1700) and principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708).

ITR4561970: La Colonnade in the Parc du Chateau de Versailles (Les Yvelines), 1660-1700. Gardens of Andre Le Notre (1613-1700) and principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708). / Bridgeman Images

ID: ITR4561970

La Colonnade in the Parc du Chateau de Versailles (Les Yvelines), 1660-1700. Gardens of Andre Le Notre (1613-1700) and principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708).

Apollo basin. Chateau de Versailles (Les Yvelines), 1660-1700. Gardens of Andre Le Notre (1613-1700) and principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708).
Apollo basin. Chateau de Versailles (Les Yvelines), 1660-1700. Gardens of Andre Le Notre (1613-1700) and principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708).

ITR4562018: Apollo basin. Chateau de Versailles (Les Yvelines), 1660-1700. Gardens of Andre Le Notre (1613-1700) and principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708). / Bridgeman Images

ID: ITR4562018

Apollo basin. Chateau de Versailles (Les Yvelines), 1660-1700. Gardens of Andre Le Notre (1613-1700) and principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708).

Office staircase, Gallimard and youth in Paris, realized in 1989 by Gonzales and Leonard. Photography 10/06/89
Office staircase, Gallimard and youth in Paris, realized in 1989 by Gonzales and Leonard. Photography 10/06/89

TEC4557216: Office staircase, Gallimard and youth in Paris, realized in 1989 by Gonzales and Leonard. Photography 10/06/89 / Bridgeman Images

ID: TEC4557216

Office staircase, Gallimard and youth in Paris, realized in 1989 by Gonzales and Leonard. Photography 10/06/89

Graphic effect, Centre de radiologie, Pau, Pyrenees-Atlantiques (Pyrenees Altantiques), Aquitaine. Architecture by Jean Jacques Cachau, 1991
Graphic effect, Centre de radiologie, Pau, Pyrenees-Atlantiques (Pyrenees Altantiques), Aquitaine. Architecture by Jean Jacques Cachau, 1991

TEC4557220: Graphic effect, Centre de radiologie, Pau, Pyrenees-Atlantiques (Pyrenees Altantiques), Aquitaine. Architecture by Jean Jacques Cachau, 1991 / Bridgeman Images

ID: TEC4557220

Graphic effect, Centre de radiologie, Pau, Pyrenees-Atlantiques (Pyrenees Altantiques), Aquitaine. Architecture by Jean Jacques Cachau, 1991

The Musee Saint-Pierre in Lyon, 1992. Renovation: Jean-Michel Wilmotte and Philippe Dubois in 1992. Photography 25/06/92
The Musee Saint-Pierre in Lyon, 1992. Renovation: Jean-Michel Wilmotte and Philippe Dubois in 1992. Photography 25/06/92

TEC4557230: The Musee Saint-Pierre in Lyon, 1992. Renovation: Jean-Michel Wilmotte and Philippe Dubois in 1992. Photography 25/06/92 / Bridgeman Images

ID: TEC4557230

The Musee Saint-Pierre in Lyon, 1992. Renovation: Jean-Michel Wilmotte and Philippe Dubois in 1992. Photography 25/06/92

Urban display in Paris, Bache overlooking the peripheric boulevard at the height of the Porte de la Chapelle, Paris 75018. Photography 01/03/01
Urban display in Paris, Bache overlooking the peripheric boulevard at the height of the Porte de la Chapelle, Paris 75018. Photography 01/03/01

TEC4557353: Urban display in Paris, Bache overlooking the peripheric boulevard at the height of the Porte de la Chapelle, Paris 75018. Photography 01/03/01 / Bridgeman Images

ID: TEC4557353

Urban display in Paris, Bache overlooking the peripheric boulevard at the height of the Porte de la Chapelle, Paris 75018. Photography 01/03/01

Urban display in Paris, Bache overlooking the peripheric boulevard at the height of the Porte de la Chapelle, Paris 75018. Photography 01/03/01
Urban display in Paris, Bache overlooking the peripheric boulevard at the height of the Porte de la Chapelle, Paris 75018. Photography 01/03/01

TEC4557356: Urban display in Paris, Bache overlooking the peripheric boulevard at the height of the Porte de la Chapelle, Paris 75018. Photography 01/03/01 / Bridgeman Images

ID: TEC4557356

Urban display in Paris, Bache overlooking the peripheric boulevard at the height of the Porte de la Chapelle, Paris 75018. Photography 01/03/01

Accommodation in Paris 13, 1984 (photo)
Accommodation in Paris 13, 1984 (photo)

TEC4557392: Accommodation in Paris 13, 1984 (photo) / Bridgeman Images

ID: TEC4557392

Accommodation in Paris 13, 1984 (photo)

Double glazing window in Paris
Double glazing window in Paris

TEC4557427: Double glazing window in Paris / Bridgeman Images

ID: TEC4557427

Double glazing window in Paris

Painted wall, Paris
Painted wall, Paris

TEC4557527: Painted wall, Paris / Bridgeman Images

ID: TEC4557527

Painted wall, Paris

Wall painted along the railways, Paris 17
Wall painted along the railways, Paris 17

TEC4557543: Wall painted along the railways, Paris 17 / Bridgeman Images

ID: TEC4557543

Wall painted along the railways, Paris 17

Wall painted in Paris
Wall painted in Paris

TEC4557560: Wall painted in Paris / Bridgeman Images

ID: TEC4557560

Wall painted in Paris

Wall painted by Le Gac, Paris 20.
Wall painted by Le Gac, Paris 20.

TEC4557563: Wall painted by Le Gac, Paris 20. / Bridgeman Images

ID: TEC4557563

Wall painted by Le Gac, Paris 20.

Villa Adrienne, 19 avenue du General Leclerc in Paris. Set up in 1780, this villa was originally intended to receive military and ecclesiastic.
Villa Adrienne, 19 avenue du General Leclerc in Paris. Set up in 1780, this villa was originally intended to receive military and ecclesiastic.

TEC4572060: Villa Adrienne, 19 avenue du General Leclerc in Paris. Set up in 1780, this villa was originally intended to receive military and ecclesiastic. / Bridgeman Images

ID: TEC4572060

Villa Adrienne, 19 avenue du General Leclerc in Paris. Set up in 1780, this villa was originally intended to receive military and ecclesiastic.

The former American Center in Paris.
The former American Center in Paris.

TEC4572167: The former American Center in Paris. / Bridgeman Images

ID: TEC4572167

The former American Center in Paris.

Workshop of sculptor Arnold Huggler (1894-1988), Villa Seurat in Paris. Construction 1925, architect Andre Lurcat (1894-1970). Impasse privee lotie in the twenty years to receive villas of artists close to Montparnasse. Photography 10/05/88.
Workshop of sculptor Arnold Huggler (1894-1988), Villa Seurat in Paris. Construction 1925, architect Andre Lurcat (1894-1970). Impasse privee lotie in the twenty years to receive villas of artists close to Montparnasse. Photography 10/05/88.

TEC4572200: Workshop of sculptor Arnold Huggler (1894-1988), Villa Seurat in Paris. Construction 1925, architect Andre Lurcat (1894-1970). Impasse privee lotie in the twenty years to receive villas of artists close to Montparnasse. Photography 10/05/88. / Bridgeman Images

ID: TEC4572200

Workshop of sculptor Arnold Huggler (1894-1988), Villa Seurat in Paris. Construction 1925, architect Andre Lurcat (1894-1970). Impasse privee lotie in the twenty years to receive villas of artists close to Montparnasse. Photography 10/05/88.


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