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Via Ravecca, Genoa, Liguria, Italy
Via Ravecca, Genoa, Liguria, Italy

CUB4540427: Via Ravecca, Genoa, Liguria, Italy / Bridgeman Images

ID: CUB4540427

Via Ravecca, Genoa, Liguria, Italy

The arches of the apse, at the bedside of the cathedral. Notre Dame de Paris Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXeme, rehabilitation by Viollet-le-Duc -
The arches of the apse, at the bedside of the cathedral. Notre Dame de Paris Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXeme, rehabilitation by Viollet-le-Duc -

ITR4553930: The arches of the apse, at the bedside of the cathedral. Notre Dame de Paris Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXeme, rehabilitation by Viollet-le-Duc - / Bridgeman Images

ID: ITR4553930

The arches of the apse, at the bedside of the cathedral. Notre Dame de Paris Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXeme, rehabilitation by Viollet-le-Duc -

Notre Dame de Lorette, neighborhood Richelieu Drouot, Paris 9th.
Notre Dame de Lorette, neighborhood Richelieu Drouot, Paris 9th.

TEC4618331: Notre Dame de Lorette, neighborhood Richelieu Drouot, Paris 9th. / Bridgeman Images

ID: TEC4618331

Notre Dame de Lorette, neighborhood Richelieu Drouot, Paris 9th.

View of the chapels built from the 13th century on the north coast of the nef.Cathedrale Notre Dame de Paris Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc -
View of the chapels built from the 13th century on the north coast of the nef.Cathedrale Notre Dame de Paris Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc -

ITR4553957: View of the chapels built from the 13th century on the north coast of the nef.Cathedrale Notre Dame de Paris Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc - / Bridgeman Images

ID: ITR4553957

View of the chapels built from the 13th century on the north coast of the nef.Cathedrale Notre Dame de Paris Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc -

Our Lady invites to contemplation. Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc -
Our Lady invites to contemplation. Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc -

ITR4553984: Our Lady invites to contemplation. Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc - / Bridgeman Images

ID: ITR4553984

Our Lady invites to contemplation. Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc -

L'Opera Garnier, Place de l'Opera, Paris 9th. Architect Charles Garnier, construction 1862-1875. The Opera or the National Academy of Music and Dance represents the best architectural expression of the Napoleon III style, eclectic, baroque, overload. Photography 2002.
L'Opera Garnier, Place de l'Opera, Paris 9th. Architect Charles Garnier, construction 1862-1875. The Opera or the National Academy of Music and Dance represents the best architectural expression of the Napoleon III style, eclectic, baroque, overload. Photography 2002.

LBY4618499: L'Opera Garnier, Place de l'Opera, Paris 9th. Architect Charles Garnier, construction 1862-1875. The Opera or the National Academy of Music and Dance represents the best architectural expression of the Napoleon III style, eclectic, baroque, overload. Photography 2002. / Bridgeman Images

ID: LBY4618499

L'Opera Garnier, Place de l'Opera, Paris 9th. Architect Charles Garnier, construction 1862-1875. The Opera or the National Academy of Music and Dance represents the best architectural expression of the Napoleon III style, eclectic, baroque, overload. Photography 2002.

Blind repacking simulating a window with four lancets adjacent to the south rose: it is an eloquent witness to the refinement of Pierre de Montreuil's art, around 1260. Notre Dame de Paris Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXeme, rehabilitation by Viollet-le-Duc -
Blind repacking simulating a window with four lancets adjacent to the south rose: it is an eloquent witness to the refinement of Pierre de Montreuil's art, around 1260. Notre Dame de Paris Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXeme, rehabilitation by Viollet-le-Duc -

ITR4554081: Blind repacking simulating a window with four lancets adjacent to the south rose: it is an eloquent witness to the refinement of Pierre de Montreuil's art, around 1260. Notre Dame de Paris Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXeme, rehabilitation by Viollet-le-Duc - / Bridgeman Images

ID: ITR4554081

Blind repacking simulating a window with four lancets adjacent to the south rose: it is an eloquent witness to the refinement of Pierre de Montreuil's art, around 1260. Notre Dame de Paris Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXeme, rehabilitation by Viollet-le-Duc -

L'Hotel de la Paiva, Place Saint Georges, Paris 9th. Architect Edouard Renaud, construction 1840. Photography 2002.
L'Hotel de la Paiva, Place Saint Georges, Paris 9th. Architect Edouard Renaud, construction 1840. Photography 2002.

LBY4618545: L'Hotel de la Paiva, Place Saint Georges, Paris 9th. Architect Edouard Renaud, construction 1840. Photography 2002. / Bridgeman Images

ID: LBY4618545

L'Hotel de la Paiva, Place Saint Georges, Paris 9th. Architect Edouard Renaud, construction 1840. Photography 2002.

Buildings in Libertini street, Lecce, Puglia, Italy
Buildings in Libertini street, Lecce, Puglia, Italy

CUB4541467: Buildings in Libertini street, Lecce, Puglia, Italy / Bridgeman Images

ID: CUB4541467

Buildings in Libertini street, Lecce, Puglia, Italy

Scene in Libertini street, Lecce, Puglia, Italy
Scene in Libertini street, Lecce, Puglia, Italy

CUB4541503: Scene in Libertini street, Lecce, Puglia, Italy / Bridgeman Images

ID: CUB4541503

Scene in Libertini street, Lecce, Puglia, Italy

Nebula NGC 7023 in Cephee - Iris Nebula in Cepheus - The nebula of the Iris (NGC 7023) is a reflexion nebula illuminated by the star HD 200775. Infrared observations indicate that this nebula contains PAH (aromatic polycyclic hydrocarbons), molecules composed of carbon atoms and hydrogen. NGC 7023 (The Iris Nebula) is located 1400 Light Years away. The bright star HD 200775 shining through the nebula NGC 7023 is a 10 solar mass star centrally imbedded in a region surrounded by ambient molecular cloud material. Infrared observations indicate that this nebula may contain complex carbon molecules known as PaHS
Nebula NGC 7023 in Cephee - Iris Nebula in Cepheus - The nebula of the Iris (NGC 7023) is a reflexion nebula illuminated by the star HD 200775. Infrared observations indicate that this nebula contains PAH (aromatic polycyclic hydrocarbons), molecules composed of carbon atoms and hydrogen. NGC 7023 (The Iris Nebula) is located 1400 Light Years away. The bright star HD 200775 shining through the nebula NGC 7023 is a 10 solar mass star centrally imbedded in a region surrounded by ambient molecular cloud material. Infrared observations indicate that this nebula may contain complex carbon molecules known as PaHS

PIX4620553: Nebula NGC 7023 in Cephee - Iris Nebula in Cepheus - The nebula of the Iris (NGC 7023) is a reflexion nebula illuminated by the star HD 200775. Infrared observations indicate that this nebula contains PAH (aromatic polycyclic hydrocarbons), molecules composed of carbon atoms and hydrogen. NGC 7023 (The Iris Nebula) is located 1400 Light Years away. The bright star HD 200775 shining through the nebula NGC 7023 is a 10 solar mass star centrally imbedded in a region surrounded by ambient molecular cloud material. Infrared observations indicate that this nebula may contain complex carbon molecules known as PaHS / Bridgeman Images

ID: PIX4620553

Nebula NGC 7023 in Cephee - Iris Nebula in Cepheus - The nebula of the Iris (NGC 7023) is a reflexion nebula illuminated by the star HD 200775. Infrared observations indicate that this nebula contains PAH (aromatic polycyclic hydrocarbons), molecules composed of carbon atoms and hydrogen. NGC 7023 (The Iris Nebula) is located 1400 Light Years away. The bright star HD 200775 shining through the nebula NGC 7023 is a 10 solar mass star centrally imbedded in a region surrounded by ambient molecular cloud material. Infrared observations indicate that this nebula may contain complex carbon molecules known as PaHS

Nebula NGC 7538 in Cassiopee - Nebula NGC 7538 in Cassiopeia - NGC 7538 is about 7000 light years away in the constellation Cepheus
Nebula NGC 7538 in Cassiopee - Nebula NGC 7538 in Cassiopeia - NGC 7538 is about 7000 light years away in the constellation Cepheus

PIX4620610: Nebula NGC 7538 in Cassiopee - Nebula NGC 7538 in Cassiopeia - NGC 7538 is about 7000 light years away in the constellation Cepheus / Bridgeman Images

ID: PIX4620610

Nebula NGC 7538 in Cassiopee - Nebula NGC 7538 in Cassiopeia - NGC 7538 is about 7000 light years away in the constellation Cepheus

Friedrichstrasse Station, Mitte Quarter aae Berlin (Germany).
Friedrichstrasse Station, Mitte Quarter aae Berlin (Germany).

LBY4620719: Friedrichstrasse Station, Mitte Quarter aae Berlin (Germany). / Bridgeman Images

ID: LBY4620719

Friedrichstrasse Station, Mitte Quarter aae Berlin (Germany).

The Brandenburg Gate in Berlin (Germany). Architecteae Carl Gotthard Langhans, 1791. Photography 10/10/99.
The Brandenburg Gate in Berlin (Germany). Architecteae Carl Gotthard Langhans, 1791. Photography 10/10/99.

LBY4620793: The Brandenburg Gate in Berlin (Germany). Architecteae Carl Gotthard Langhans, 1791. Photography 10/10/99. / Bridgeman Images

ID: LBY4620793

The Brandenburg Gate in Berlin (Germany). Architecteae Carl Gotthard Langhans, 1791. Photography 10/10/99.

Field around the Nebula Henize 55 - The Henize 55 star forming region in the LMC - Henize 55 (NGC 2014), on the right, is a star-forming region located north of the Great Magellan Cloud. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. The nearby Large Magellanic Cloud (LMC) is a very active star - forming galaxy. The most massive region of star formation is around 30 Doradus (the Tarantula nebula) which can be seen with the unaided eye, but hundreds of lesser examples are visible with a telescope. This picture shows one of the more intriguing, NGC 2014 (Henize 55), at right. It contains cluster of hot, young stars, almost hidden in the brightest part of the nebula. The energetic ultraviolet light from these stars is absorbed by hydrogen and produces the distinctive red glow from an enormous distance around the cluster. This picture was made photographically from three glass plates taken with the UK Schmidt telescope of Siding Spring
Field around the Nebula Henize 55 - The Henize 55 star forming region in the LMC - Henize 55 (NGC 2014), on the right, is a star-forming region located north of the Great Magellan Cloud. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. The nearby Large Magellanic Cloud (LMC) is a very active star - forming galaxy. The most massive region of star formation is around 30 Doradus (the Tarantula nebula) which can be seen with the unaided eye, but hundreds of lesser examples are visible with a telescope. This picture shows one of the more intriguing, NGC 2014 (Henize 55), at right. It contains cluster of hot, young stars, almost hidden in the brightest part of the nebula. The energetic ultraviolet light from these stars is absorbed by hydrogen and produces the distinctive red glow from an enormous distance around the cluster. This picture was made photographically from three glass plates taken with the UK Schmidt telescope of Siding Spring

PIX4620819: Field around the Nebula Henize 55 - The Henize 55 star forming region in the LMC - Henize 55 (NGC 2014), on the right, is a star-forming region located north of the Great Magellan Cloud. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. The nearby Large Magellanic Cloud (LMC) is a very active star - forming galaxy. The most massive region of star formation is around 30 Doradus (the Tarantula nebula) which can be seen with the unaided eye, but hundreds of lesser examples are visible with a telescope. This picture shows one of the more intriguing, NGC 2014 (Henize 55), at right. It contains cluster of hot, young stars, almost hidden in the brightest part of the nebula. The energetic ultraviolet light from these stars is absorbed by hydrogen and produces the distinctive red glow from an enormous distance around the cluster. This picture was made photographically from three glass plates taken with the UK Schmidt telescope of Siding Spring / Bridgeman Images

ID: PIX4620819

Field around the Nebula Henize 55 - The Henize 55 star forming region in the LMC - Henize 55 (NGC 2014), on the right, is a star-forming region located north of the Great Magellan Cloud. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. The nearby Large Magellanic Cloud (LMC) is a very active star - forming galaxy. The most massive region of star formation is around 30 Doradus (the Tarantula nebula) which can be seen with the unaided eye, but hundreds of lesser examples are visible with a telescope. This picture shows one of the more intriguing, NGC 2014 (Henize 55), at right. It contains cluster of hot, young stars, almost hidden in the brightest part of the nebula. The energetic ultraviolet light from these stars is absorbed by hydrogen and produces the distinctive red glow from an enormous distance around the cluster. This picture was made photographically from three glass plates taken with the UK Schmidt telescope of Siding Spring

Galerie Victor Emmanuel II in Milan, Italy. Architect Giuseppe Mengoni (1829-1877).
Galerie Victor Emmanuel II in Milan, Italy. Architect Giuseppe Mengoni (1829-1877).

TEC4620880: Galerie Victor Emmanuel II in Milan, Italy. Architect Giuseppe Mengoni (1829-1877). / Bridgeman Images

ID: TEC4620880

Galerie Victor Emmanuel II in Milan, Italy. Architect Giuseppe Mengoni (1829-1877).

Taurus Molecular Cloud - Taurus Molecular Cloud - This region is located on the border of the Taurus and Persee constellations. Covering about 20 x 30 degres, this image shows a complex of emitted nebulae, star clusters, reflexion nebulae and dark nebulae. A molecular cloud is a region of dense gas and dust composed mainly of molecular hydrogen and helium. It's a birthplace of stars. The Molecular Cloud of Taurus is located about 400 years ago - light, and is one of the closest molecular clouds to our solar system. The California Nebula (NGC 1499), an emission nebula located about 1000 years ago - is visible at the top right. The dark nebulae B7, B18 and B19 are visible near the center of the image. Les Pleiades, M45, is the open cluster at the bottom right center. The open clusters NGC 1817, NGC 1746, NGC 1647 are on the left side of the image. The Hyades, Melotte 25, is a V-shaped cluster at the bottom left. It is the closest open cluster, located at a distance of about 151 light years. Aldebaran, Alpha Tauri, a bright red star with a magnitude of 0.75 to 0.95, is located at one end of the V, but does not belong to the cluster. The Taurus Molecular Cloud (TMC) is located on the border of the constellations of Taurus and Perseus. It is a large dense area of gas and dust in space made mostly of molecular hydrogen and helium. It is a birth place of stars, which form from the material in the cloud. Covering about 20 x 30 degrees, this wide - angle image shows a complex of bright red emission nebulae, star clusters, blue reflection nebulosity, and complex dark nebulae. The TMC is located about 400 light years away, and is one of the closest molecular clouds to our solar system. The California Nebula (NGC 1499), a very large red emission nebula, is at upper right. Emission nebulae are made up of glowing hydrogen gas. Located in
Taurus Molecular Cloud - Taurus Molecular Cloud - This region is located on the border of the Taurus and Persee constellations. Covering about 20 x 30 degres, this image shows a complex of emitted nebulae, star clusters, reflexion nebulae and dark nebulae. A molecular cloud is a region of dense gas and dust composed mainly of molecular hydrogen and helium. It's a birthplace of stars. The Molecular Cloud of Taurus is located about 400 years ago - light, and is one of the closest molecular clouds to our solar system. The California Nebula (NGC 1499), an emission nebula located about 1000 years ago - is visible at the top right. The dark nebulae B7, B18 and B19 are visible near the center of the image. Les Pleiades, M45, is the open cluster at the bottom right center. The open clusters NGC 1817, NGC 1746, NGC 1647 are on the left side of the image. The Hyades, Melotte 25, is a V-shaped cluster at the bottom left. It is the closest open cluster, located at a distance of about 151 light years. Aldebaran, Alpha Tauri, a bright red star with a magnitude of 0.75 to 0.95, is located at one end of the V, but does not belong to the cluster. The Taurus Molecular Cloud (TMC) is located on the border of the constellations of Taurus and Perseus. It is a large dense area of gas and dust in space made mostly of molecular hydrogen and helium. It is a birth place of stars, which form from the material in the cloud. Covering about 20 x 30 degrees, this wide - angle image shows a complex of bright red emission nebulae, star clusters, blue reflection nebulosity, and complex dark nebulae. The TMC is located about 400 light years away, and is one of the closest molecular clouds to our solar system. The California Nebula (NGC 1499), a very large red emission nebula, is at upper right. Emission nebulae are made up of glowing hydrogen gas. Located in

PIX4621177: Taurus Molecular Cloud - Taurus Molecular Cloud - This region is located on the border of the Taurus and Persee constellations. Covering about 20 x 30 degres, this image shows a complex of emitted nebulae, star clusters, reflexion nebulae and dark nebulae. A molecular cloud is a region of dense gas and dust composed mainly of molecular hydrogen and helium. It's a birthplace of stars. The Molecular Cloud of Taurus is located about 400 years ago - light, and is one of the closest molecular clouds to our solar system. The California Nebula (NGC 1499), an emission nebula located about 1000 years ago - is visible at the top right. The dark nebulae B7, B18 and B19 are visible near the center of the image. Les Pleiades, M45, is the open cluster at the bottom right center. The open clusters NGC 1817, NGC 1746, NGC 1647 are on the left side of the image. The Hyades, Melotte 25, is a V-shaped cluster at the bottom left. It is the closest open cluster, located at a distance of about 151 light years. Aldebaran, Alpha Tauri, a bright red star with a magnitude of 0.75 to 0.95, is located at one end of the V, but does not belong to the cluster. The Taurus Molecular Cloud (TMC) is located on the border of the constellations of Taurus and Perseus. It is a large dense area of gas and dust in space made mostly of molecular hydrogen and helium. It is a birth place of stars, which form from the material in the cloud. Covering about 20 x 30 degrees, this wide - angle image shows a complex of bright red emission nebulae, star clusters, blue reflection nebulosity, and complex dark nebulae. The TMC is located about 400 light years away, and is one of the closest molecular clouds to our solar system. The California Nebula (NGC 1499), a very large red emission nebula, is at upper right. Emission nebulae are made up of glowing hydrogen gas. Located in / Bridgeman Images

ID: PIX4621177

Taurus Molecular Cloud - Taurus Molecular Cloud - This region is located on the border of the Taurus and Persee constellations. Covering about 20 x 30 degres, this image shows a complex of emitted nebulae, star clusters, reflexion nebulae and dark nebulae. A molecular cloud is a region of dense gas and dust composed mainly of molecular hydrogen and helium. It's a birthplace of stars. The Molecular Cloud of Taurus is located about 400 years ago - light, and is one of the closest molecular clouds to our solar system. The California Nebula (NGC 1499), an emission nebula located about 1000 years ago - is visible at the top right. The dark nebulae B7, B18 and B19 are visible near the center of the image. Les Pleiades, M45, is the open cluster at the bottom right center. The open clusters NGC 1817, NGC 1746, NGC 1647 are on the left side of the image. The Hyades, Melotte 25, is a V-shaped cluster at the bottom left. It is the closest open cluster, located at a distance of about 151 light yea

Nebulae B175 and VDB 152 in Cephee - Nebulae B175 and VDB 152 in Cephe
Nebulae B175 and VDB 152 in Cephee - Nebulae B175 and VDB 152 in Cephe

PIX4621230: Nebulae B175 and VDB 152 in Cephee - Nebulae B175 and VDB 152 in Cephe / Bridgeman Images

ID: PIX4621230

Nebulae B175 and VDB 152 in Cephee - Nebulae B175 and VDB 152 in Cephe

Piazza Duomo with the cathedral, Lecce, Puglia, Italy
Piazza Duomo with the cathedral, Lecce, Puglia, Italy

CUB4541536: Piazza Duomo with the cathedral, Lecce, Puglia, Italy / Bridgeman Images

ID: CUB4541536

Piazza Duomo with the cathedral, Lecce, Puglia, Italy

Villa La Meridiana, Santa Maria di Leuca, Salento, Puglia, Italy
Villa La Meridiana, Santa Maria di Leuca, Salento, Puglia, Italy

CUB4541557: Villa La Meridiana, Santa Maria di Leuca, Salento, Puglia, Italy / Bridgeman Images

ID: CUB4541557

Villa La Meridiana, Santa Maria di Leuca, Salento, Puglia, Italy

The ancient core of the city as seen from the sky, Gallipoli, Salento, Puglia, Italy
The ancient core of the city as seen from the sky, Gallipoli, Salento, Puglia, Italy

CUB4541629: The ancient core of the city as seen from the sky, Gallipoli, Salento, Puglia, Italy / Bridgeman Images

ID: CUB4541629

The ancient core of the city as seen from the sky, Gallipoli, Salento, Puglia, Italy

Typical shape (Paiara) in the country, Salento, Puglia, Italy
Typical shape (Paiara) in the country, Salento, Puglia, Italy

CUB4541692: Typical shape (Paiara) in the country, Salento, Puglia, Italy / Bridgeman Images

ID: CUB4541692

Typical shape (Paiara) in the country, Salento, Puglia, Italy

San Foca, Salento, Puglia, Italy
San Foca, Salento, Puglia, Italy

CUB4541698: San Foca, Salento, Puglia, Italy / Bridgeman Images

ID: CUB4541698

San Foca, Salento, Puglia, Italy

Torre Miggiano, Salento, Puglia, Italy
Torre Miggiano, Salento, Puglia, Italy

CUB4541701: Torre Miggiano, Salento, Puglia, Italy / Bridgeman Images

ID: CUB4541701

Torre Miggiano, Salento, Puglia, Italy

Specchia, Salento, Puglia, Italy
Specchia, Salento, Puglia, Italy

CUB4541719: Specchia, Salento, Puglia, Italy / Bridgeman Images

ID: CUB4541719

Specchia, Salento, Puglia, Italy

Olives, Salento, Puglia, Italy
Olives, Salento, Puglia, Italy

CUB4541753: Olives, Salento, Puglia, Italy / Bridgeman Images

ID: CUB4541753

Olives, Salento, Puglia, Italy

Aragonese castle, Otranto, Salento, Puglia, Italy
Aragonese castle, Otranto, Salento, Puglia, Italy

CUB4541768: Aragonese castle, Otranto, Salento, Puglia, Italy / Bridgeman Images

ID: CUB4541768

Aragonese castle, Otranto, Salento, Puglia, Italy

Otranto, Salento, Puglia, Italy
Otranto, Salento, Puglia, Italy

CUB4541780: Otranto, Salento, Puglia, Italy / Bridgeman Images

ID: CUB4541780

Otranto, Salento, Puglia, Italy

La Place Gambetta in Paris 20th. Photogaphie 26/08/07.
La Place Gambetta in Paris 20th. Photogaphie 26/08/07.

TEC4616597: La Place Gambetta in Paris 20th. Photogaphie 26/08/07. / Bridgeman Images

ID: TEC4616597

La Place Gambetta in Paris 20th. Photogaphie 26/08/07.

Saint Sulpice Church (Saint Sulpice), Place Saint Sulpice, Paris 6 (France). Architect Jean Nicolas Servandoni, 1646-1780.
Saint Sulpice Church (Saint Sulpice), Place Saint Sulpice, Paris 6 (France). Architect Jean Nicolas Servandoni, 1646-1780.

TEC4552707: Saint Sulpice Church (Saint Sulpice), Place Saint Sulpice, Paris 6 (France). Architect Jean Nicolas Servandoni, 1646-1780. / Bridgeman Images

ID: TEC4552707

Saint Sulpice Church (Saint Sulpice), Place Saint Sulpice, Paris 6 (France). Architect Jean Nicolas Servandoni, 1646-1780.

View over the Castello Aragonese, Ischia, Campania, Italy
View over the Castello Aragonese, Ischia, Campania, Italy

CUB4539700: View over the Castello Aragonese, Ischia, Campania, Italy / Bridgeman Images

ID: CUB4539700

View over the Castello Aragonese, Ischia, Campania, Italy

Sitting at the City Hall for the Palio, Siena, Tuscany, Italy
Sitting at the City Hall for the Palio, Siena, Tuscany, Italy

CUB4539733: Sitting at the City Hall for the Palio, Siena, Tuscany, Italy / Bridgeman Images

ID: CUB4539733

Sitting at the City Hall for the Palio, Siena, Tuscany, Italy

silhouette, Siena, Tuscany, Italy
silhouette, Siena, Tuscany, Italy

CUB4539769: silhouette, Siena, Tuscany, Italy / Bridgeman Images

ID: CUB4539769

silhouette, Siena, Tuscany, Italy

Celebrations after the victory inside the Cathedral, Siena, Tuscany, Italy
Celebrations after the victory inside the Cathedral, Siena, Tuscany, Italy

CUB4539778: Celebrations after the victory inside the Cathedral, Siena, Tuscany, Italy / Bridgeman Images

ID: CUB4539778

Celebrations after the victory inside the Cathedral, Siena, Tuscany, Italy

Piazza Duomo and the cathedral, Catania, The baroque in Sicily, Italy
Piazza Duomo and the cathedral, Catania, The baroque in Sicily, Italy

CUB4539796: Piazza Duomo and the cathedral, Catania, The baroque in Sicily, Italy / Bridgeman Images

ID: CUB4539796

Piazza Duomo and the cathedral, Catania, The baroque in Sicily, Italy

Palazzo Biscari, Catania, The Baroque in Sicily, Italy
Palazzo Biscari, Catania, The Baroque in Sicily, Italy

CUB4539823: Palazzo Biscari, Catania, The Baroque in Sicily, Italy / Bridgeman Images

ID: CUB4539823

Palazzo Biscari, Catania, The Baroque in Sicily, Italy


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