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L'alsace Heureé: Le pont du Rhine à Brisach (print)
L'alsace Heureé: Le pont du Rhine à Brisach (print)

JLJ4622347: L'alsace Heureé: Le pont du Rhine à Brisach (print), Waltz, Jean-Jacques (Hansi) (1873-1951) / Bridgeman Images

L'alsace Heureé: La ronde enfantine à Guemar (print)
L'alsace Heureé: La ronde enfantine à Guemar (print)

JLJ4622367: L'alsace Heureé: La ronde enfantine à Guemar (print), Waltz, Jean-Jacques (Hansi) (1873-1951) / Bridgeman Images

Marche de la rue Mouffetard in Paris.
Marche de la rue Mouffetard in Paris.

TEC4622414: Marche de la rue Mouffetard in Paris. / Bridgeman Images

The story of Alsace tells the children: Cesar et ses legions (print)
The story of Alsace tells the children: Cesar et ses legions (print)

JLJ4622422: The story of Alsace tells the children: Cesar et ses legions (print), Waltz, Jean-Jacques (Hansi) (1873-1951) / Bridgeman Images

Detail in nebula IC 1848 in Cassiopee - Detail in nebula IC 1848 in Cassiope
Detail in nebula IC 1848 in Cassiopee - Detail in nebula IC 1848 in Cassiope

PIX4622449: Detail in nebula IC 1848 in Cassiopee - Detail in nebula IC 1848 in Cassiope / Bridgeman Images

Urban signage between Boulevard Saint Michel and Boulevard Saint Germain, Paris 5e.
Urban signage between Boulevard Saint Michel and Boulevard Saint Germain, Paris 5e.

TEC4622464: Urban signage between Boulevard Saint Michel and Boulevard Saint Germain, Paris 5e. / Bridgeman Images

Jesus in the house of Martha and Mary of Bethany, 1620 (painting)
Jesus in the house of Martha and Mary of Bethany, 1620 (painting)

LRI4622483: Jesus in the house of Martha and Mary of Bethany, 1620 (painting), Steenwyk, Hendrik van (the Younger) (c.1580-1649) / Bridgeman Images

Representation of the actor Arashi Toyozo c.1794 (print)
Representation of the actor Arashi Toyozo c.1794 (print)

JLJ4564674: Representation of the actor Arashi Toyozo c.1794 (print), Sharaku, Toshusai (fl.1794-95) / Bridgeman Images

Representation of actor Nakamura Shikan IV. Japanese print of the 19th century (print)
Representation of actor Nakamura Shikan IV. Japanese print of the 19th century (print)

JLJ4564705: Representation of actor Nakamura Shikan IV. Japanese print of the 19th century (print), Japanese School, (19th century) / Bridgeman Images

Globular cluster M10 in Ophiuchus - Globular Cluster M10 - M10 (NGC 6254) is a globular cluster of magnitude 7 located about 15,000 years - light from Earth in the constellation Ophiuchus. Image obtained by the Hubble Space Telescope (HST). M10, or NGC 6254, is a seventh magnitude globular cluster in the constellation Ophiuchus, close to M12. About 15000 light - years away and about 70 light - years across, M10 on the sky has about half the diameter of the full moon. This image is made up of observations made in visible and infrared light using Hubble's Advanced Camera for Surveys
Globular cluster M10 in Ophiuchus - Globular Cluster M10 - M10 (NGC 6254) is a globular cluster of magnitude 7 located about 15,000 years - light from Earth in the constellation Ophiuchus. Image obtained by the Hubble Space Telescope (HST). M10, or NGC 6254, is a seventh magnitude globular cluster in the constellation Ophiuchus, close to M12. About 15000 light - years away and about 70 light - years across, M10 on the sky has about half the diameter of the full moon. This image is made up of observations made in visible and infrared light using Hubble's Advanced Camera for Surveys

PIX4564731: Globular cluster M10 in Ophiuchus - Globular Cluster M10 - M10 (NGC 6254) is a globular cluster of magnitude 7 located about 15,000 years - light from Earth in the constellation Ophiuchus. Image obtained by the Hubble Space Telescope (HST). M10, or NGC 6254, is a seventh magnitude globular cluster in the constellation Ophiuchus, close to M12. About 15000 light - years away and about 70 light - years across, M10 on the sky has about half the diameter of the full moon. This image is made up of observations made in visible and infrared light using Hubble's Advanced Camera for Surveys / Bridgeman Images

Globular clusters M9 and NGC 6356 in Ophiuchus - Globular clusters M9 and NGC 6356 in Ophiuchus - Globular clusters M9 (NGC 6333, right) and NGC 6356 (top). M9 is one of the closest globular clusters to the center of our galaxy. NGC 6356 is twice as far away from us, about 50,000 years of light from Earth. Globular clusters M9 (NGC 6333), on the right and NGC 6356, on the top. M9 is one of the nearer globular clusters to the center of our Galaxy. NGC 6356 is two times distant from us, at about 50,000 light years
Globular clusters M9 and NGC 6356 in Ophiuchus - Globular clusters M9 and NGC 6356 in Ophiuchus - Globular clusters M9 (NGC 6333, right) and NGC 6356 (top). M9 is one of the closest globular clusters to the center of our galaxy. NGC 6356 is twice as far away from us, about 50,000 years of light from Earth. Globular clusters M9 (NGC 6333), on the right and NGC 6356, on the top. M9 is one of the nearer globular clusters to the center of our Galaxy. NGC 6356 is two times distant from us, at about 50,000 light years

PIX4564747: Globular clusters M9 and NGC 6356 in Ophiuchus - Globular clusters M9 and NGC 6356 in Ophiuchus - Globular clusters M9 (NGC 6333, right) and NGC 6356 (top). M9 is one of the closest globular clusters to the center of our galaxy. NGC 6356 is twice as far away from us, about 50,000 years of light from Earth. Globular clusters M9 (NGC 6333), on the right and NGC 6356, on the top. M9 is one of the nearer globular clusters to the center of our Galaxy. NGC 6356 is two times distant from us, at about 50,000 light years / Bridgeman Images

Globular cluster M92 in Hercules - Globular cluster M92 in Hercules - M92 is a cluster of stars located about 28,000 light years away from Earth in the constellation Hercules. M92 is a globular cluster at a distance of about 28,000 light - years away from Earth in the Hercules constellation
Globular cluster M92 in Hercules - Globular cluster M92 in Hercules - M92 is a cluster of stars located about 28,000 light years away from Earth in the constellation Hercules. M92 is a globular cluster at a distance of about 28,000 light - years away from Earth in the Hercules constellation

PIX4564771: Globular cluster M92 in Hercules - Globular cluster M92 in Hercules - M92 is a cluster of stars located about 28,000 light years away from Earth in the constellation Hercules. M92 is a globular cluster at a distance of about 28,000 light - years away from Earth in the Hercules constellation / Bridgeman Images

Globular cluster M14 in Ophiuchus - Globular cluster M14 in the constellation Ophiuchus - The globular cluster M14 is located in the constellation Ophiuchus at a distance of about 29,000 years - light; it extends over 72 years - light. M14 is a somewhat looser globular cluster than many, with a very small ellipticity (deviation from being exactly circular on the sky). Appearing in the constellation Ophiuchus, it is about 29000 light - years away and about 72 light - years across
Globular cluster M14 in Ophiuchus - Globular cluster M14 in the constellation Ophiuchus - The globular cluster M14 is located in the constellation Ophiuchus at a distance of about 29,000 years - light; it extends over 72 years - light. M14 is a somewhat looser globular cluster than many, with a very small ellipticity (deviation from being exactly circular on the sky). Appearing in the constellation Ophiuchus, it is about 29000 light - years away and about 72 light - years across

PIX4564838: Globular cluster M14 in Ophiuchus - Globular cluster M14 in the constellation Ophiuchus - The globular cluster M14 is located in the constellation Ophiuchus at a distance of about 29,000 years - light; it extends over 72 years - light. M14 is a somewhat looser globular cluster than many, with a very small ellipticity (deviation from being exactly circular on the sky). Appearing in the constellation Ophiuchus, it is about 29000 light - years away and about 72 light - years across / Bridgeman Images

Portrait of Sergei Rachmaninov (b/w photo)
Portrait of Sergei Rachmaninov (b/w photo)

LRI4564887: Portrait of Sergei Rachmaninov (b/w photo), Unknown photographer, (20th century) / Bridgeman Images

Globular cluster M54 in Sagittarius - Globular cluster M54 in Sagittarius - The globular cluster M54 photographed by the Hubble space telescope (HST). M54 resides about 90,000 light years from Earth, in the dwarf galaxy of Sagittarius. The object shown in this beautiful Hubble image, dubbed Messier 54, could be just another globular cluster, but this dense and faint group of stars was in fact the first globular cluster found that is outside our galaxy. Discovered by the famous astronomer Charles Messier in 1778, Messier 54 belongs to a satellite of the Milky Way called the Sagittarius Dwarf Elliptical Galaxy. Messier had no idea of the significance of his discovery at the time, and it wasn't until over two centuries later, in 1994, that astronomers found Messier 54 to be part of the miniature galaxy and not our own. Current estimates indicate that the Sagittarius dwarf, and hence the cluster, is situated almost 90 000 light - years away - - more than three times as far from the centre of our galaxy than the Solar System. Ironically, even though this globular cluster is now understood to lie outside the Milky Way, it will actually become part of it in the future. The strong gravitational pull of our galaxy is slowly engulfing the Sagittarius dwarf, which will eventually merge with the Milky Way creating one much larger galaxy. This picture is a composite created by combining images taken with the Wide Field Channel of Hubble's Advanced Camera for Surveys. Light that passed through a yellow - orange (F606W) was colored blue and light passing through a near - infrared filter (F814W) was colored red. The total exposure times were 3460 s and 3560 s, respectively and the field of view is approximately 3.4 by 3.4 arcminutes
Globular cluster M54 in Sagittarius - Globular cluster M54 in Sagittarius - The globular cluster M54 photographed by the Hubble space telescope (HST). M54 resides about 90,000 light years from Earth, in the dwarf galaxy of Sagittarius. The object shown in this beautiful Hubble image, dubbed Messier 54, could be just another globular cluster, but this dense and faint group of stars was in fact the first globular cluster found that is outside our galaxy. Discovered by the famous astronomer Charles Messier in 1778, Messier 54 belongs to a satellite of the Milky Way called the Sagittarius Dwarf Elliptical Galaxy. Messier had no idea of the significance of his discovery at the time, and it wasn't until over two centuries later, in 1994, that astronomers found Messier 54 to be part of the miniature galaxy and not our own. Current estimates indicate that the Sagittarius dwarf, and hence the cluster, is situated almost 90 000 light - years away - - more than three times as far from the centre of our galaxy than the Solar System. Ironically, even though this globular cluster is now understood to lie outside the Milky Way, it will actually become part of it in the future. The strong gravitational pull of our galaxy is slowly engulfing the Sagittarius dwarf, which will eventually merge with the Milky Way creating one much larger galaxy. This picture is a composite created by combining images taken with the Wide Field Channel of Hubble's Advanced Camera for Surveys. Light that passed through a yellow - orange (F606W) was colored blue and light passing through a near - infrared filter (F814W) was colored red. The total exposure times were 3460 s and 3560 s, respectively and the field of view is approximately 3.4 by 3.4 arcminutes

PIX4565011: Globular cluster M54 in Sagittarius - Globular cluster M54 in Sagittarius - The globular cluster M54 photographed by the Hubble space telescope (HST). M54 resides about 90,000 light years from Earth, in the dwarf galaxy of Sagittarius. The object shown in this beautiful Hubble image, dubbed Messier 54, could be just another globular cluster, but this dense and faint group of stars was in fact the first globular cluster found that is outside our galaxy. Discovered by the famous astronomer Charles Messier in 1778, Messier 54 belongs to a satellite of the Milky Way called the Sagittarius Dwarf Elliptical Galaxy. Messier had no idea of the significance of his discovery at the time, and it wasn't until over two centuries later, in 1994, that astronomers found Messier 54 to be part of the miniature galaxy and not our own. Current estimates indicate that the Sagittarius dwarf, and hence the cluster, is situated almost 90 000 light - years away - - more than three times as far from the centre of our galaxy than the Solar System. Ironically, even though this globular cluster is now understood to lie outside the Milky Way, it will actually become part of it in the future. The strong gravitational pull of our galaxy is slowly engulfing the Sagittarius dwarf, which will eventually merge with the Milky Way creating one much larger galaxy. This picture is a composite created by combining images taken with the Wide Field Channel of Hubble's Advanced Camera for Surveys. Light that passed through a yellow - orange (F606W) was colored blue and light passing through a near - infrared filter (F814W) was colored red. The total exposure times were 3460 s and 3560 s, respectively and the field of view is approximately 3.4 by 3.4 arcminutes / Bridgeman Images

Night end - Starry sky and observer - Constellations of the Great Bear, Lion and Cancer 26 September 2006, Monts d'Arree (Finistere - France). In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. Big Dipper, Leo, Cancer constellations. Mythological Constellations forms from “” Uranographia”” star atlas by Hevelius (1690) have been added. September 26 2006, Monts d'Arree (Finistere - France)
Night end - Starry sky and observer - Constellations of the Great Bear, Lion and Cancer 26 September 2006, Monts d'Arree (Finistere - France). In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. Big Dipper, Leo, Cancer constellations. Mythological Constellations forms from “” Uranographia”” star atlas by Hevelius (1690) have been added. September 26 2006, Monts d'Arree (Finistere - France)

PIX4592089: Night end - Starry sky and observer - Constellations of the Great Bear, Lion and Cancer 26 September 2006, Monts d'Arree (Finistere - France). In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. Big Dipper, Leo, Cancer constellations. Mythological Constellations forms from “” Uranographia”” star atlas by Hevelius (1690) have been added. September 26 2006, Monts d'Arree (Finistere - France) / Bridgeman Images

Constellation Leo - Leo constellation - The constellation of the Lion above the Chapel of Mount Saint - Michel of Braspart, Brittany. April 2008, Mont Saint - Michel de Braspart, Brittany, France)
Constellation Leo - Leo constellation - The constellation of the Lion above the Chapel of Mount Saint - Michel of Braspart, Brittany. April 2008, Mont Saint - Michel de Braspart, Brittany, France)

PIX4592104: Constellation Leo - Leo constellation - The constellation of the Lion above the Chapel of Mount Saint - Michel of Braspart, Brittany. April 2008, Mont Saint - Michel de Braspart, Brittany, France) / Bridgeman Images

Horsemen and couplers on the avenue du bois in Paris Au fond l'arc de Triomphe, 20th century (oil on canvas)
Horsemen and couplers on the avenue du bois in Paris Au fond l'arc de Triomphe, 20th century (oil on canvas)

JLJ4592153: Horsemen and couplers on the avenue du bois in Paris Au fond l'arc de Triomphe, 20th century (oil on canvas), Stein, Georges (1818-90) / Bridgeman Images

Lynx Constellation - Constellation of Lynx - Mirror of Urania by Jehoshaphat Aspin 1825 Recolorated by us Urania's Mirror, by Jehoshaphat Aspin, 1825. Recolored
Lynx Constellation - Constellation of Lynx - Mirror of Urania by Jehoshaphat Aspin 1825 Recolorated by us Urania's Mirror, by Jehoshaphat Aspin, 1825. Recolored

PIX4592224: Lynx Constellation - Constellation of Lynx - Mirror of Urania by Jehoshaphat Aspin 1825 Recolorated by us Urania's Mirror, by Jehoshaphat Aspin, 1825. Recolored / Bridgeman Images

Lyra Constellation - Constellation of Lyra - Lyra Constellation extracted from Hevelius Uranographia. Recolorised image. Map showing the constellation of Lyra with its mythological form from “” Uranographia”” star atlas by Hevelius (1690). Recolored Image
Lyra Constellation - Constellation of Lyra - Lyra Constellation extracted from Hevelius Uranographia. Recolorised image. Map showing the constellation of Lyra with its mythological form from “” Uranographia”” star atlas by Hevelius (1690). Recolored Image

PIX4592270: Lyra Constellation - Constellation of Lyra - Lyra Constellation extracted from Hevelius Uranographia. Recolorised image. Map showing the constellation of Lyra with its mythological form from “” Uranographia”” star atlas by Hevelius (1690). Recolored Image / Bridgeman Images

Vedado district in Havana, Cuba.
Vedado district in Havana, Cuba.

TEC4592321: Vedado district in Havana, Cuba. / Bridgeman Images

Centro Habana district in Havana, Cuba.
Centro Habana district in Havana, Cuba.

TEC4592391: Centro Habana district in Havana, Cuba. / Bridgeman Images

The story of Alsace tells the children: Construction of a cathedrale (print)
The story of Alsace tells the children: Construction of a cathedrale (print)

JLJ4622493: The story of Alsace tells the children: Construction of a cathedrale (print), Waltz, Jean-Jacques (Hansi) (1873-1951) / 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

Eglise Notre Dame du Val de Grace (1624-1669) in Paris. The church is the fruit of the wish of Queen Anne of Austria to raise a beautiful temple to God if he sent her a son. After twenty-three years of marriage, in 1638, the future Louis XIV was born, who laid the first stone on 1 April 1645 and the construction ended at the end of the 1660s with sculptural and pictorial decoration. The works were first entrusted to Mansart, to which Le Mercier was succeeded, having worked notably at the Hotel de St Aignan and the Bibliotheque of Mazarin, and then Le Muet, who attended Le Duc. In 1649, the disturbances of the Fronde led to a long interruption of work, which did not resume until 1655. Photography 10/08/98.
Eglise Notre Dame du Val de Grace (1624-1669) in Paris. The church is the fruit of the wish of Queen Anne of Austria to raise a beautiful temple to God if he sent her a son. After twenty-three years of marriage, in 1638, the future Louis XIV was born, who laid the first stone on 1 April 1645 and the construction ended at the end of the 1660s with sculptural and pictorial decoration. The works were first entrusted to Mansart, to which Le Mercier was succeeded, having worked notably at the Hotel de St Aignan and the Bibliotheque of Mazarin, and then Le Muet, who attended Le Duc. In 1649, the disturbances of the Fronde led to a long interruption of work, which did not resume until 1655. Photography 10/08/98.

TEC4622513: Eglise Notre Dame du Val de Grace (1624-1669) in Paris. The church is the fruit of the wish of Queen Anne of Austria to raise a beautiful temple to God if he sent her a son. After twenty-three years of marriage, in 1638, the future Louis XIV was born, who laid the first stone on 1 April 1645 and the construction ended at the end of the 1660s with sculptural and pictorial decoration. The works were first entrusted to Mansart, to which Le Mercier was succeeded, having worked notably at the Hotel de St Aignan and the Bibliotheque of Mazarin, and then Le Muet, who attended Le Duc. In 1649, the disturbances of the Fronde led to a long interruption of work, which did not resume until 1655. Photography 10/08/98. / Bridgeman Images

The story of Alsace tells the children: Louis XIV in Alsace (print)
The story of Alsace tells the children: Louis XIV in Alsace (print)

JLJ4622521: The story of Alsace tells the children: Louis XIV in Alsace (print), Waltz, Jean-Jacques (Hansi) (1873-1951) / Bridgeman Images

Nebula IC 2948 in Centaur - Bok's cells - A group of Bok globules in IC 2948 - View of a detail of nebula IC 2948 in the center Centaur on Bok's cells. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. The dark spots in the picture are not photographic defects but an unusual type of interstellar cloud known as a Bok globule. Bok globules, named after astronomer Bart Bok who studied them extensively, are small dark clouds made of gas and dust that are typically condensing to form a star or stars. These Bok globules are located at a distance of about 6000 light years near IC 2944 cluster in the emission nebula IC 2948
Nebula IC 2948 in Centaur - Bok's cells - A group of Bok globules in IC 2948 - View of a detail of nebula IC 2948 in the center Centaur on Bok's cells. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. The dark spots in the picture are not photographic defects but an unusual type of interstellar cloud known as a Bok globule. Bok globules, named after astronomer Bart Bok who studied them extensively, are small dark clouds made of gas and dust that are typically condensing to form a star or stars. These Bok globules are located at a distance of about 6000 light years near IC 2944 cluster in the emission nebula IC 2948

PIX4622532: Nebula IC 2948 in Centaur - Bok's cells - A group of Bok globules in IC 2948 - View of a detail of nebula IC 2948 in the center Centaur on Bok's cells. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. The dark spots in the picture are not photographic defects but an unusual type of interstellar cloud known as a Bok globule. Bok globules, named after astronomer Bart Bok who studied them extensively, are small dark clouds made of gas and dust that are typically condensing to form a star or stars. These Bok globules are located at a distance of about 6000 light years near IC 2944 cluster in the emission nebula IC 2948 / Bridgeman Images

Nebulae IC 2948 and 2944 in Centaur
Nebulae IC 2948 and 2944 in Centaur

PIX4622553: Nebulae IC 2948 and 2944 in Centaur / Bridgeman Images

Lucien Germain Guitry and Jeanne Granier, 1895 (oil on paper)
Lucien Germain Guitry and Jeanne Granier, 1895 (oil on paper)

LRI4622598: Lucien Germain Guitry and Jeanne Granier, 1895 (oil on paper), Toulouse-Lautrec, Henri de (1864-1901) / Bridgeman Images

Nebula IC 4601 in Scorpio - IC 4601 nebula in Scorpius - IC 4601 is a reflexion nebula located in the constellation Scorpio. Reflection nebula in Scorpius
Nebula IC 4601 in Scorpio - IC 4601 nebula in Scorpius - IC 4601 is a reflexion nebula located in the constellation Scorpio. Reflection nebula in Scorpius

PIX4622601: Nebula IC 4601 in Scorpio - IC 4601 nebula in Scorpius - IC 4601 is a reflexion nebula located in the constellation Scorpio. Reflection nebula in Scorpius / Bridgeman Images

Boulevard Saint Michel in Paris.
Boulevard Saint Michel in Paris.

TEC4622610: Boulevard Saint Michel in Paris. / Bridgeman Images

The story of Alsace tells the children: War of Revolution (print)
The story of Alsace tells the children: War of Revolution (print)

JLJ4622621: The story of Alsace tells the children: War of Revolution (print), Waltz, Jean-Jacques (Hansi) (1873-1951) / Bridgeman Images

The Pantheon in Paris. Construction 1757-1790, architect Jacques Germain Soufflot (1713-1780). In 1744 Louis XV, suffering from a serious illness in Metz, would wish to erect an immense church instead of the abbey of Sainte Genevieve, which was then in ruins. When the war came, he kept his word and assigned the architect Soufflot the task of drawing the plans of the monument. A great admirer of Greek Roman architecture, he imagined a gigantic building, built on a plan of Greek cross 110 metres long, 84 metres wide and 83 metres high. At the time, the project seemed so insane that many, in the court and in the salons of the capital, would question Soufflot's abilities and prevent the collapse of the monument. Louis XV confirmed his confidence in the architect and laid the foundation stone in 1764 during a grand ceremony. In 1806, the Pantheon, like all the churches in France closed during the revolution, was restored to its original name of Sainte Genevieve church. Renamed Pantheon in 1830, the building regained its vocation as a laique and patriotic temple. Headquarters to the insurgents of the Commune in 1871, during which Milliere was shot on the steps, the building was definitively transformed into a Republican monument in 1885, during the funeral of Victor Hugo.
The Pantheon in Paris. Construction 1757-1790, architect Jacques Germain Soufflot (1713-1780). In 1744 Louis XV, suffering from a serious illness in Metz, would wish to erect an immense church instead of the abbey of Sainte Genevieve, which was then in ruins. When the war came, he kept his word and assigned the architect Soufflot the task of drawing the plans of the monument. A great admirer of Greek Roman architecture, he imagined a gigantic building, built on a plan of Greek cross 110 metres long, 84 metres wide and 83 metres high. At the time, the project seemed so insane that many, in the court and in the salons of the capital, would question Soufflot's abilities and prevent the collapse of the monument. Louis XV confirmed his confidence in the architect and laid the foundation stone in 1764 during a grand ceremony. In 1806, the Pantheon, like all the churches in France closed during the revolution, was restored to its original name of Sainte Genevieve church. Renamed Pantheon in 1830, the building regained its vocation as a laique and patriotic temple. Headquarters to the insurgents of the Commune in 1871, during which Milliere was shot on the steps, the building was definitively transformed into a Republican monument in 1885, during the funeral of Victor Hugo.

TEC4622655: The Pantheon in Paris. Construction 1757-1790, architect Jacques Germain Soufflot (1713-1780). In 1744 Louis XV, suffering from a serious illness in Metz, would wish to erect an immense church instead of the abbey of Sainte Genevieve, which was then in ruins. When the war came, he kept his word and assigned the architect Soufflot the task of drawing the plans of the monument. A great admirer of Greek Roman architecture, he imagined a gigantic building, built on a plan of Greek cross 110 metres long, 84 metres wide and 83 metres high. At the time, the project seemed so insane that many, in the court and in the salons of the capital, would question Soufflot's abilities and prevent the collapse of the monument. Louis XV confirmed his confidence in the architect and laid the foundation stone in 1764 during a grand ceremony. In 1806, the Pantheon, like all the churches in France closed during the revolution, was restored to its original name of Sainte Genevieve church. Renamed Pantheon in 1830, the building regained its vocation as a laique and patriotic temple. Headquarters to the insurgents of the Commune in 1871, during which Milliere was shot on the steps, the building was definitively transformed into a Republican monument in 1885, during the funeral of Victor Hugo. / Bridgeman Images

The tricolor paradise: The Place du Marche in Thann, 1918 (print)
The tricolor paradise: The Place du Marche in Thann, 1918 (print)

JLJ4622691: The tricolor paradise: The Place du Marche in Thann, 1918 (print), Waltz, Jean-Jacques (Hansi) (1873-1951) / Bridgeman Images

Napoleonic War:
Napoleonic War:

JLJ4622696: Napoleonic War: "The French infantry against the Prussian cavalry", 19th century (watercolour), Unknown Artist, (19th century) / Bridgeman Images

The tricolor paradise: At the border (print)
The tricolor paradise: At the border (print)

JLJ4622712: The tricolor paradise: At the border (print), Waltz, Jean-Jacques (Hansi) (1873-1951) / Bridgeman Images


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