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Nebulae B175 and VDB 152 in Cephee - Nebulae B175 and VDB 152 in Cephee - In the center of the picture, a large dust trail leads to a blue nebula. This is the dark nebula, Barnard 175, which coaches the nebula by reflexion VDB 152 (Ced 201). The image is oriented with the North on the left. Image obtained with Takahashi 180 Astrograph telescope and Apogee U9 camera
Nebulae B175 and VDB 152 in Cephee - Nebulae B175 and VDB 152 in Cephee - In the center of the picture, a large dust trail leads to a blue nebula. This is the dark nebula, Barnard 175, which coaches the nebula by reflexion VDB 152 (Ced 201). The image is oriented with the North on the left. Image obtained with Takahashi 180 Astrograph telescope and Apogee U9 camera

PIX4621233: Nebulae B175 and VDB 152 in Cephee - Nebulae B175 and VDB 152 in Cephee - In the center of the picture, a large dust trail leads to a blue nebula. This is the dark nebula, Barnard 175, which coaches the nebula by reflexion VDB 152 (Ced 201). The image is oriented with the North on the left. Image obtained with Takahashi 180 Astrograph telescope and Apogee U9 camera / Bridgeman Images

ID: PIX4621233

Nebulae B175 and VDB 152 in Cephee - Nebulae B175 and VDB 152 in Cephee - In the center of the picture, a large dust trail leads to a blue nebula. This is the dark nebula, Barnard 175, which coaches the nebula by reflexion VDB 152 (Ced 201). The image is oriented with the North on the left. Image obtained with Takahashi 180 Astrograph telescope and Apogee U9 camera

Seaport with the Embarkation of Saint Ursula (oil on canvas, 1641)
Seaport with the Embarkation of Saint Ursula (oil on canvas, 1641)

LRI4621346: Seaport with the Embarkation of Saint Ursula (oil on canvas, 1641), Le Lorrain, Louis-Joseph (1715-59) / Bridgeman Images

ID: LRI4621346

Seaport with the Embarkation of Saint Ursula (oil on canvas, 1641)

Le Lorrain, Louis-Joseph (1715-59)

Nebulae LBN 552 and Cohen 129 - Nebulae LBN 552 and Cohen 129 in Cepheus - Nebulae in the constellation Cephee. This region in Cepheus does offer delicate reflection nebulae that have been cataloged by Beverly T. Lynds, University of Arizona, in 1965. This catalog was made from studying the red and blue plates taken by the 48 - inch Palomar Sky Survey. Cohen 129 is the small yellow nebula just slightly up of center
Nebulae LBN 552 and Cohen 129 - Nebulae LBN 552 and Cohen 129 in Cepheus - Nebulae in the constellation Cephee. This region in Cepheus does offer delicate reflection nebulae that have been cataloged by Beverly T. Lynds, University of Arizona, in 1965. This catalog was made from studying the red and blue plates taken by the 48 - inch Palomar Sky Survey. Cohen 129 is the small yellow nebula just slightly up of center

PIX4621422: Nebulae LBN 552 and Cohen 129 - Nebulae LBN 552 and Cohen 129 in Cepheus - Nebulae in the constellation Cephee. This region in Cepheus does offer delicate reflection nebulae that have been cataloged by Beverly T. Lynds, University of Arizona, in 1965. This catalog was made from studying the red and blue plates taken by the 48 - inch Palomar Sky Survey. Cohen 129 is the small yellow nebula just slightly up of center / Bridgeman Images

ID: PIX4621422

Nebulae LBN 552 and Cohen 129 - Nebulae LBN 552 and Cohen 129 in Cepheus - Nebulae in the constellation Cephee. This region in Cepheus does offer delicate reflection nebulae that have been cataloged by Beverly T. Lynds, University of Arizona, in 1965. This catalog was made from studying the red and blue plates taken by the 48 - inch Palomar Sky Survey. Cohen 129 is the small yellow nebula just slightly up of center

Saint Paul and Saint Dominic. Polyptych of Orvieto (tempera and gold on panel, 1321)
Saint Paul and Saint Dominic. Polyptych of Orvieto (tempera and gold on panel, 1321)

LRI4621450: Saint Paul and Saint Dominic. Polyptych of Orvieto (tempera and gold on panel, 1321), Martini, Simone (1284-1344) / Bridgeman Images

ID: LRI4621450

Saint Paul and Saint Dominic. Polyptych of Orvieto (tempera and gold on panel, 1321)

Martini, Simone (1284-1344)

Cometary blood cell CG4 in the stern - CG4, a cometary blood cell in Puppis - Cometary blood cells are small clouds of isolated gases. The latter, called CG4, is located about 1300 light years ago in the constellation of Pupus. Its head is 1.5 years light and its tail extends for 8 years. This cloud is a star-forming region. A spiral galaxy seen by the slice (ESO 257 - 19) is visible at the top left. It is located 100 million years later. The odd looking “” creature”” to the right of center in the above photo is a gas cloud known as a cometary globule.This globule, however, has ruptured. Cometary globules are typically characterized by dusty heads and elongated tails. These features cause cometary globules to have visual similarities to comets, but in reality they are very much different. Cometary globules are frequently the birthplaces of stars, and many show very young stars in their heads. The reason for the rupture in the head of this object is not completely known. The galaxy to the left of center is very far in the distance and is only placed near CG4 by chance superposition
Cometary blood cell CG4 in the stern - CG4, a cometary blood cell in Puppis - Cometary blood cells are small clouds of isolated gases. The latter, called CG4, is located about 1300 light years ago in the constellation of Pupus. Its head is 1.5 years light and its tail extends for 8 years. This cloud is a star-forming region. A spiral galaxy seen by the slice (ESO 257 - 19) is visible at the top left. It is located 100 million years later. The odd looking “” creature”” to the right of center in the above photo is a gas cloud known as a cometary globule.This globule, however, has ruptured. Cometary globules are typically characterized by dusty heads and elongated tails. These features cause cometary globules to have visual similarities to comets, but in reality they are very much different. Cometary globules are frequently the birthplaces of stars, and many show very young stars in their heads. The reason for the rupture in the head of this object is not completely known. The galaxy to the left of center is very far in the distance and is only placed near CG4 by chance superposition

PIX4621547: Cometary blood cell CG4 in the stern - CG4, a cometary blood cell in Puppis - Cometary blood cells are small clouds of isolated gases. The latter, called CG4, is located about 1300 light years ago in the constellation of Pupus. Its head is 1.5 years light and its tail extends for 8 years. This cloud is a star-forming region. A spiral galaxy seen by the slice (ESO 257 - 19) is visible at the top left. It is located 100 million years later. The odd looking “” creature”” to the right of center in the above photo is a gas cloud known as a cometary globule.This globule, however, has ruptured. Cometary globules are typically characterized by dusty heads and elongated tails. These features cause cometary globules to have visual similarities to comets, but in reality they are very much different. Cometary globules are frequently the birthplaces of stars, and many show very young stars in their heads. The reason for the rupture in the head of this object is not completely known. The galaxy to the left of center is very far in the distance and is only placed near CG4 by chance superposition / Bridgeman Images

ID: PIX4621547

Cometary blood cell CG4 in the stern - CG4, a cometary blood cell in Puppis - Cometary blood cells are small clouds of isolated gases. The latter, called CG4, is located about 1300 light years ago in the constellation of Pupus. Its head is 1.5 years light and its tail extends for 8 years. This cloud is a star-forming region. A spiral galaxy seen by the slice (ESO 257 - 19) is visible at the top left. It is located 100 million years later. The odd looking “” creature”” to the right of center in the above photo is a gas cloud known as a cometary globule.This globule, however, has ruptured. Cometary globules are typically characterized by dusty heads and elongated tails. These features cause cometary globules to have visual similarities to comets, but in reality they are very much different. Cometary globules are frequently the birthplaces of stars, and many show very young stars in their heads. The reason for the rupture in the head of this object is not completely known. The galaxy to t

Dante's boat, from Divina Commedia by Dante Alighieri (oil on canvas, 1822)
Dante's boat, from Divina Commedia by Dante Alighieri (oil on canvas, 1822)

LRI4620876: Dante's boat, from Divina Commedia by Dante Alighieri (oil on canvas, 1822), Delacroix, Ferdinand Victor Eugene (1798-1863) / Bridgeman Images

ID: LRI4620876

Dante's boat, from Divina Commedia by Dante Alighieri (oil on canvas, 1822)

Delacroix, Ferdinand Victor Eugene (1798-1863)

Henry IV (1553-1610) at the fair of Saint Germain, after his marriage, December 16, 1600, 1907 (illustration)
Henry IV (1553-1610) at the fair of Saint Germain, after his marriage, December 16, 1600, 1907 (illustration)

JLJ4620870: Henry IV (1553-1610) at the fair of Saint Germain, after his marriage, December 16, 1600, 1907 (illustration), Vogel, Hermann (1856-1918) / Bridgeman Images

ID: JLJ4620870

Henry IV (1553-1610) at the fair of Saint Germain, after his marriage, December 16, 1600, 1907 (illustration)

Vogel, Hermann (1856-1918)

Reception of Charles V (1500-1558), King of Spain and Emperor of the Holy Roman Empire, to Amboise, in 1540, 1909 (illustration)
Reception of Charles V (1500-1558), King of Spain and Emperor of the Holy Roman Empire, to Amboise, in 1540, 1909 (illustration)

JLJ4621037: Reception of Charles V (1500-1558), King of Spain and Emperor of the Holy Roman Empire, to Amboise, in 1540, 1909 (illustration), Robida, Albert (1848-1926) / Bridgeman Images

ID: JLJ4621037

Reception of Charles V (1500-1558), King of Spain and Emperor of the Holy Roman Empire, to Amboise, in 1540, 1909 (illustration)

Robida, Albert (1848-1926)

Pieright of the right-hand portal of the western facade of the Basilica of Saint Denis, France (photo)
Pieright of the right-hand portal of the western facade of the Basilica of Saint Denis, France (photo)

JLJ4621260: Pieright of the right-hand portal of the western facade of the Basilica of Saint Denis, France (photo), French School / Bridgeman Images

ID: JLJ4621260

Pieright of the right-hand portal of the western facade of the Basilica of Saint Denis, France (photo)

French School

Nebula Sh2 - 261 in Orion - Image based on data obtained with the Oschin telescope of Mount Palomar
Nebula Sh2 - 261 in Orion - Image based on data obtained with the Oschin telescope of Mount Palomar

PIX4621118: Nebula Sh2 - 261 in Orion - Image based on data obtained with the Oschin telescope of Mount Palomar / Bridgeman Images

ID: PIX4621118

Nebula Sh2 - 261 in Orion - Image based on data obtained with the Oschin telescope of Mount Palomar

Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star-forming region is about 6200 years old - light. Hidden in light visible by interstellar dust, this region rises in infrared light. Gas filaments appear in red; they emphasize the presence of aromatic polycyclic hydrocarbons (PAH); they are organic molecules composed of carbon atoms and hydrogen that could be the germs on which the first bricks of life appeared. Image obtained by the Spitzer space telescope in 2003. Hidden behind a shroud of dust in the constellation Cygnus is a stellar nursery called DR21, which is giving birth to some of the most massive stars in our galaxy. Visible light images reveal no trace of this interstellar cauldron because of heavy dust obscuration. This image from Nasa's Spitzer Space Telescope allow us to peek behind the cosmic veil and pinpoint one of the most massive natal stars yet seen in our Milky Way galaxy. The never - before - seen star is 100,000 times as bright as the Sun. Also revealed for the first time is a powerful outflow of hot gas emanating from this star and bursting through a giant molecular cloud. The image is a large - scale mosaic assembled from individual photographs obtained with the Infraared Array Camera (IRAC) aboard Spitzer. The image covers an area about two times that of a full moon. The mosaic is a composite of images obtained at mid - infrared wavelengths of 3.6 microns (blue), 4.5 microns (green), 5.8 microns (orange) and 8 microns (red). The brightest infrared cloud near the top center corresponds to DR21, which presumably contains a cluster of newly forming stars at a distance of 10,000 light - years. Protruding out from DR21 toward the bottom left of the image is a gaseous outflow (green), containing both carbon monoxide and molecular hydrogen. Data from the Spitzer spectrograph, which breaks light into its constitutes
Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star-forming region is about 6200 years old - light. Hidden in light visible by interstellar dust, this region rises in infrared light. Gas filaments appear in red; they emphasize the presence of aromatic polycyclic hydrocarbons (PAH); they are organic molecules composed of carbon atoms and hydrogen that could be the germs on which the first bricks of life appeared. Image obtained by the Spitzer space telescope in 2003. Hidden behind a shroud of dust in the constellation Cygnus is a stellar nursery called DR21, which is giving birth to some of the most massive stars in our galaxy. Visible light images reveal no trace of this interstellar cauldron because of heavy dust obscuration. This image from Nasa's Spitzer Space Telescope allow us to peek behind the cosmic veil and pinpoint one of the most massive natal stars yet seen in our Milky Way galaxy. The never - before - seen star is 100,000 times as bright as the Sun. Also revealed for the first time is a powerful outflow of hot gas emanating from this star and bursting through a giant molecular cloud. The image is a large - scale mosaic assembled from individual photographs obtained with the Infraared Array Camera (IRAC) aboard Spitzer. The image covers an area about two times that of a full moon. The mosaic is a composite of images obtained at mid - infrared wavelengths of 3.6 microns (blue), 4.5 microns (green), 5.8 microns (orange) and 8 microns (red). The brightest infrared cloud near the top center corresponds to DR21, which presumably contains a cluster of newly forming stars at a distance of 10,000 light - years. Protruding out from DR21 toward the bottom left of the image is a gaseous outflow (green), containing both carbon monoxide and molecular hydrogen. Data from the Spitzer spectrograph, which breaks light into its constitutes

PIX4621130: Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star-forming region is about 6200 years old - light. Hidden in light visible by interstellar dust, this region rises in infrared light. Gas filaments appear in red; they emphasize the presence of aromatic polycyclic hydrocarbons (PAH); they are organic molecules composed of carbon atoms and hydrogen that could be the germs on which the first bricks of life appeared. Image obtained by the Spitzer space telescope in 2003. Hidden behind a shroud of dust in the constellation Cygnus is a stellar nursery called DR21, which is giving birth to some of the most massive stars in our galaxy. Visible light images reveal no trace of this interstellar cauldron because of heavy dust obscuration. This image from Nasa's Spitzer Space Telescope allow us to peek behind the cosmic veil and pinpoint one of the most massive natal stars yet seen in our Milky Way galaxy. The never - before - seen star is 100,000 times as bright as the Sun. Also revealed for the first time is a powerful outflow of hot gas emanating from this star and bursting through a giant molecular cloud. The image is a large - scale mosaic assembled from individual photographs obtained with the Infraared Array Camera (IRAC) aboard Spitzer. The image covers an area about two times that of a full moon. The mosaic is a composite of images obtained at mid - infrared wavelengths of 3.6 microns (blue), 4.5 microns (green), 5.8 microns (orange) and 8 microns (red). The brightest infrared cloud near the top center corresponds to DR21, which presumably contains a cluster of newly forming stars at a distance of 10,000 light - years. Protruding out from DR21 toward the bottom left of the image is a gaseous outflow (green), containing both carbon monoxide and molecular hydrogen. Data from the Spitzer spectrograph, which breaks light into its constitutes / Bridgeman Images

ID: PIX4621130

Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star-forming region is about 6200 years old - light. Hidden in light visible by interstellar dust, this region rises in infrared light. Gas filaments appear in red; they emphasize the presence of aromatic polycyclic hydrocarbons (PAH); they are organic molecules composed of carbon atoms and hydrogen that could be the germs on which the first bricks of life appeared. Image obtained by the Spitzer space telescope in 2003. Hidden behind a shroud of dust in the constellation Cygnus is a stellar nursery called DR21, which is giving birth to some of the most massive stars in our galaxy. Visible light images reveal no trace of this interstellar cauldron because of heavy dust obscuration. This image from Nasa's Spitzer Space Telescope allow us to peek behind the cosmic veil and pinpoint one of the most massive natal stars yet seen in our Milky Way galaxy. The never - before - seen star is 100,000 times as bright as th

Nebuleuse Sh2 - 142 in Cephee - Nebuleuse Sh2 - 142 in Cephee - Region of star formation in Cephee and star clusters NGC 7380
Nebuleuse Sh2 - 142 in Cephee - Nebuleuse Sh2 - 142 in Cephee - Region of star formation in Cephee and star clusters NGC 7380

PIX4621043: Nebuleuse Sh2 - 142 in Cephee - Nebuleuse Sh2 - 142 in Cephee - Region of star formation in Cephee and star clusters NGC 7380 / Bridgeman Images

ID: PIX4621043

Nebuleuse Sh2 - 142 in Cephee - Nebuleuse Sh2 - 142 in Cephee - Region of star formation in Cephee and star clusters NGC 7380

King Francois I taken prisoner in Pavia in 1525 after fighting attackers, 1909 (Illustration)
King Francois I taken prisoner in Pavia in 1525 after fighting attackers, 1909 (Illustration)

JLJ4621124: King Francois I taken prisoner in Pavia in 1525 after fighting attackers, 1909 (Illustration), Robida, Albert (1848-1926) / Bridgeman Images

ID: JLJ4621124

King Francois I taken prisoner in Pavia in 1525 after fighting attackers, 1909 (Illustration)

Robida, Albert (1848-1926)

Pieright of the right-hand portal of the western facade of the Basilica of Saint Denis, France (photo)
Pieright of the right-hand portal of the western facade of the Basilica of Saint Denis, France (photo)

JLJ4621279: Pieright of the right-hand portal of the western facade of the Basilica of Saint Denis, France (photo), French School / Bridgeman Images

ID: JLJ4621279

Pieright of the right-hand portal of the western facade of the Basilica of Saint Denis, France (photo)

French School

Pieright of the right-hand portal of the western facade of the Basilica of Saint Denis, France (photo)
Pieright of the right-hand portal of the western facade of the Basilica of Saint Denis, France (photo)

JLJ4621292: Pieright of the right-hand portal of the western facade of the Basilica of Saint Denis, France (photo), French School / Bridgeman Images

ID: JLJ4621292

Pieright of the right-hand portal of the western facade of the Basilica of Saint Denis, France (photo)

French School

Triumph of the Republic. Paris, Place De La Nation, 1879-99 (bronze)
Triumph of the Republic. Paris, Place De La Nation, 1879-99 (bronze)

JLJ4621340: Triumph of the Republic. Paris, Place De La Nation, 1879-99 (bronze), Dalou, Aime Jules (1838-1902) / Bridgeman Images

ID: JLJ4621340

Triumph of the Republic. Paris, Place De La Nation, 1879-99 (bronze)

Dalou, Aime Jules (1838-1902)

Virgin with child, st John the baptist and st Ambrose - Altarpiece with three panel, around 1430
Virgin with child, st John the baptist and st Ambrose - Altarpiece with three panel, around 1430

LRI4621373: Virgin with child, st John the baptist and st Ambrose - Altarpiece with three panel, around 1430, Master of Burgo de Osma, (fl.1400-20) / Bridgeman Images

ID: LRI4621373

Virgin with child, st John the baptist and st Ambrose - Altarpiece with three panel, around 1430

Master of Burgo de Osma, (fl.1400-20)

Joachim & Caroline Murat hosted a party in Paris' Place Vendome, 1910 (Engraving)
Joachim & Caroline Murat hosted a party in Paris' Place Vendome, 1910 (Engraving)

JLJ4621501: Joachim & Caroline Murat hosted a party in Paris' Place Vendome, 1910 (Engraving), Job, pseudonym for Onfray de Breville, Jacques (1858-1931) / Bridgeman Images

ID: JLJ4621501

Joachim & Caroline Murat hosted a party in Paris' Place Vendome, 1910 (Engraving)

Job, pseudonym for Onfray de Breville, Jacques (1858-1931)

Virgin with child (tempera and gold on panel, 1321)
Virgin with child (tempera and gold on panel, 1321)

LRI4621439: Virgin with child (tempera and gold on panel, 1321), Martini, Simone (1284-1344) / Bridgeman Images

ID: LRI4621439

Virgin with child (tempera and gold on panel, 1321)

Martini, Simone (1284-1344)

Formation d'étoiles dans la Carene - Star formation in Carina - Region de formation d'étoiles CED 110 dans la Carene. Star - forming region CED 110 in Carina
Formation d'étoiles dans la Carene - Star formation in Carina - Region de formation d'étoiles CED 110 dans la Carene. Star - forming region CED 110 in Carina

PIX4621453: Formation d'étoiles dans la Carene - Star formation in Carina - Region de formation d'étoiles CED 110 dans la Carene. Star - forming region CED 110 in Carina / Bridgeman Images

ID: PIX4621453

Formation d'étoiles dans la Carene - Star formation in Carina - Region de formation d'étoiles CED 110 dans la Carene. Star - forming region CED 110 in Carina

In Florence, in the theatre hall, Joachim Murat (1767-1815), 1910 (engraving)
In Florence, in the theatre hall, Joachim Murat (1767-1815), 1910 (engraving)

JLJ4621489: In Florence, in the theatre hall, Joachim Murat (1767-1815), 1910 (engraving), Job, pseudonym for Onfray de Breville, Jacques (1858-1931) / Bridgeman Images

ID: JLJ4621489

In Florence, in the theatre hall, Joachim Murat (1767-1815), 1910 (engraving)

Job, pseudonym for Onfray de Breville, Jacques (1858-1931)

Diptych of Jean du Cellier: Virgin and six saints (oil on panel, 1490)
Diptych of Jean du Cellier: Virgin and six saints (oil on panel, 1490)

LRI4621494: Diptych of Jean du Cellier: Virgin and six saints (oil on panel, 1490), Memling, Hans (c.1433-94) / Bridgeman Images

ID: LRI4621494

Diptych of Jean du Cellier: Virgin and six saints (oil on panel, 1490)

Memling, Hans (c.1433-94)

Cometary blood cell CG4 in the stern - Cometary blood cell CG4 - Cometary blood cells are small clouds of isolated gases. The latter, called CG4, is located about 1300 light years ago in the constellation of Pupus. Its head is 1.5 years - light and its tail (off-field) extends for 8 years - light. This cloud is a star-forming region. Image obtained by the VLT. The cometary globule CG4 glows menacingly in this image from Eso's Very Large Telescope. Although it looks huge and bright in this image it is actually a faint nebula and not easy to observe. The exact nature of CG4 remains a mystery
Cometary blood cell CG4 in the stern - Cometary blood cell CG4 - Cometary blood cells are small clouds of isolated gases. The latter, called CG4, is located about 1300 light years ago in the constellation of Pupus. Its head is 1.5 years - light and its tail (off-field) extends for 8 years - light. This cloud is a star-forming region. Image obtained by the VLT. The cometary globule CG4 glows menacingly in this image from Eso's Very Large Telescope. Although it looks huge and bright in this image it is actually a faint nebula and not easy to observe. The exact nature of CG4 remains a mystery

PIX4621573: Cometary blood cell CG4 in the stern - Cometary blood cell CG4 - Cometary blood cells are small clouds of isolated gases. The latter, called CG4, is located about 1300 light years ago in the constellation of Pupus. Its head is 1.5 years - light and its tail (off-field) extends for 8 years - light. This cloud is a star-forming region. Image obtained by the VLT. The cometary globule CG4 glows menacingly in this image from Eso's Very Large Telescope. Although it looks huge and bright in this image it is actually a faint nebula and not easy to observe. The exact nature of CG4 remains a mystery / Bridgeman Images

ID: PIX4621573

Cometary blood cell CG4 in the stern - Cometary blood cell CG4 - Cometary blood cells are small clouds of isolated gases. The latter, called CG4, is located about 1300 light years ago in the constellation of Pupus. Its head is 1.5 years - light and its tail (off-field) extends for 8 years - light. This cloud is a star-forming region. Image obtained by the VLT. The cometary globule CG4 glows menacingly in this image from Eso's Very Large Telescope. Although it looks huge and bright in this image it is actually a faint nebula and not easy to observe. The exact nature of CG4 remains a mystery

Saints James and Ansano praying. Painting by Paolo di Dono dit Paolo Uccello (1397-1475), 1435-1440. Predelle of Quarata. Tempera on wood. Dim: 20x178cm. Florence, Museo Arcivescovile di Cestello. - Saints James and Ansano (Quarate Predella), by Paolo di Dono detto a.k.a. Paolo Uccello, (1397-1475). Tempera on wood, 20x178 cm, 1435-40. Museo Arcivescovile di Cestello, Florence, Italy
Saints James and Ansano praying. Painting by Paolo di Dono dit Paolo Uccello (1397-1475), 1435-1440. Predelle of Quarata. Tempera on wood. Dim: 20x178cm. Florence, Museo Arcivescovile di Cestello. - Saints James and Ansano (Quarate Predella), by Paolo di Dono detto a.k.a. Paolo Uccello, (1397-1475). Tempera on wood, 20x178 cm, 1435-40. Museo Arcivescovile di Cestello, Florence, Italy

LRI4621581: Saints James and Ansano praying. Painting by Paolo di Dono dit Paolo Uccello (1397-1475), 1435-1440. Predelle of Quarata. Tempera on wood. Dim: 20x178cm. Florence, Museo Arcivescovile di Cestello. - Saints James and Ansano (Quarate Predella), by Paolo di Dono detto a.k.a. Paolo Uccello, (1397-1475). Tempera on wood, 20x178 cm, 1435-40. Museo Arcivescovile di Cestello, Florence, Italy, Uccello, Paolo (1397-1475) / Bridgeman Images

ID: LRI4621581

Saints James and Ansano praying. Painting by Paolo di Dono dit Paolo Uccello (1397-1475), 1435-1440. Predelle of Quarata. Tempera on wood. Dim: 20x178cm. Florence, Museo Arcivescovile di Cestello. - Saints James and Ansano (Quarate Predella), by Paolo di Dono detto a.k.a. Paolo Uccello, (1397-1475). Tempera on wood, 20x178 cm, 1435-40. Museo Arcivescovile di Cestello, Florence, Italy

Uccello, Paolo (1397-1475)

Nebula VDB 154 in Cephee - Nebula VDB 154 in Cepheus - VDB 154 is a nebula by reflexion. Other objects visible in this field are Sh2 - 150, LBN 520, LDN 1207 - 9. Nebula reflection. Other objects visible are Sh2 - 150, LBN 520, LDN 1207 - 9
Nebula VDB 154 in Cephee - Nebula VDB 154 in Cepheus - VDB 154 is a nebula by reflexion. Other objects visible in this field are Sh2 - 150, LBN 520, LDN 1207 - 9. Nebula reflection. Other objects visible are Sh2 - 150, LBN 520, LDN 1207 - 9

PIX4621793: Nebula VDB 154 in Cephee - Nebula VDB 154 in Cepheus - VDB 154 is a nebula by reflexion. Other objects visible in this field are Sh2 - 150, LBN 520, LDN 1207 - 9. Nebula reflection. Other objects visible are Sh2 - 150, LBN 520, LDN 1207 - 9 / Bridgeman Images

ID: PIX4621793

Nebula VDB 154 in Cephee - Nebula VDB 154 in Cepheus - VDB 154 is a nebula by reflexion. Other objects visible in this field are Sh2 - 150, LBN 520, LDN 1207 - 9. Nebula reflection. Other objects visible are Sh2 - 150, LBN 520, LDN 1207 - 9

Housing building, Paris 16th.
Housing building, Paris 16th.

TEC4624122: Housing building, Paris 16th. / Bridgeman Images

ID: TEC4624122

Housing building, Paris 16th.

Grantecan dome - La Palma Observatory - Grantecan dome - La Palma observatory: dome housing the Gran Telescopio Canarias of 10.4 m
Grantecan dome - La Palma Observatory - Grantecan dome - La Palma observatory: dome housing the Gran Telescopio Canarias of 10.4 m

PIX4624160: Grantecan dome - La Palma Observatory - Grantecan dome - La Palma observatory: dome housing the Gran Telescopio Canarias of 10.4 m / Bridgeman Images

ID: PIX4624160

Grantecan dome - La Palma Observatory - Grantecan dome - La Palma observatory: dome housing the Gran Telescopio Canarias of 10.4 m

JLJ4623887: "A la gloire des betes" text, editor Maison Alfred Mame et fils: Saint Pacome et les crocodiles (illustration), Job, pseudonym for Onfray de Breville, Jacques (1858-1931) / Bridgeman Images

ID: JLJ4623887

"A la gloire des betes" text, editor Maison Alfred Mame et fils: Saint Pacome et les crocodiles (illustration)

Job, pseudonym for Onfray de Breville, Jacques (1858-1931)

View of Mercanti square with carnival scenes (oil on wood, 1850)
View of Mercanti square with carnival scenes (oil on wood, 1850)

LRI4624198: View of Mercanti square with carnival scenes (oil on wood, 1850), Guerillot Inganni, Amanzia (1828-c.1905) / Bridgeman Images

ID: LRI4624198

View of Mercanti square with carnival scenes (oil on wood, 1850)

Guerillot Inganni, Amanzia (1828-c.1905)

The Palais de Tokyo from New York Avenue in Paris. Architects: Andre Aubert, Paul Viard, Jean Claude Dondel and Marcel Dastugue, 1937. Built for the 1937 World Exhibition, the International Exhibition of Arts and Techniques in the Modern City. The Palais de Tokyo is a small part of the Luxembourg Museum and the Peure Palais too narrow to accommodate municipal collections. It owes its name to the Tokyo wharf, now New York Avenue.
The Palais de Tokyo from New York Avenue in Paris. Architects: Andre Aubert, Paul Viard, Jean Claude Dondel and Marcel Dastugue, 1937. Built for the 1937 World Exhibition, the International Exhibition of Arts and Techniques in the Modern City. The Palais de Tokyo is a small part of the Luxembourg Museum and the Peure Palais too narrow to accommodate municipal collections. It owes its name to the Tokyo wharf, now New York Avenue.

TEC4623973: The Palais de Tokyo from New York Avenue in Paris. Architects: Andre Aubert, Paul Viard, Jean Claude Dondel and Marcel Dastugue, 1937. Built for the 1937 World Exhibition, the International Exhibition of Arts and Techniques in the Modern City. The Palais de Tokyo is a small part of the Luxembourg Museum and the Peure Palais too narrow to accommodate municipal collections. It owes its name to the Tokyo wharf, now New York Avenue. / Bridgeman Images

ID: TEC4623973

The Palais de Tokyo from New York Avenue in Paris. Architects: Andre Aubert, Paul Viard, Jean Claude Dondel and Marcel Dastugue, 1937. Built for the 1937 World Exhibition, the International Exhibition of Arts and Techniques in the Modern City. The Palais de Tokyo is a small part of the Luxembourg Museum and the Peure Palais too narrow to accommodate municipal collections. It owes its name to the Tokyo wharf, now New York Avenue.

Illustration from the book
Illustration from the book

JLJ4623985: Illustration from the book "A la gloire des betes" text, publisher Maison Alfred Mame and son: The lion of Florence (illustration), Job, pseudonym for Onfray de Breville, Jacques (1858-1931) / Bridgeman Images

ID: JLJ4623985

Illustration from the book "A la gloire des betes" text, publisher Maison Alfred Mame and son: The lion of Florence (illustration)

Job, pseudonym for Onfray de Breville, Jacques (1858-1931)

Revolutions of 1848, Five Days of Milan: Austrian prisoners on Borromeo square on March 20th (painting, 19th century)
Revolutions of 1848, Five Days of Milan: Austrian prisoners on Borromeo square on March 20th (painting, 19th century)

LRI4624097: Revolutions of 1848, Five Days of Milan: Austrian prisoners on Borromeo square on March 20th (painting, 19th century), Italian School, (19th century) / Bridgeman Images

ID: LRI4624097

Revolutions of 1848, Five Days of Milan: Austrian prisoners on Borromeo square on March 20th (painting, 19th century)

Italian School, (19th century)

Passy cemetery in Paris.
Passy cemetery in Paris.

TEC4623927: Passy cemetery in Paris. / Bridgeman Images

ID: TEC4623927

Passy cemetery in Paris.

The Musee Galliera, 14 avenue du President Wilson, Paris 16th. Construction 1878-1894. Architect Leon Ginain (1825-1898). In order to give the City of Paris her art collections, the Duchess of Galliera built a museum in 1894, a pastiche of the Italian Renaissance. But for political reasons, it is the city of Genes (Italy) that houses the guilt and paintings while Paris remains the owner of this museum.
The Musee Galliera, 14 avenue du President Wilson, Paris 16th. Construction 1878-1894. Architect Leon Ginain (1825-1898). In order to give the City of Paris her art collections, the Duchess of Galliera built a museum in 1894, a pastiche of the Italian Renaissance. But for political reasons, it is the city of Genes (Italy) that houses the guilt and paintings while Paris remains the owner of this museum.

TEC4623978: The Musee Galliera, 14 avenue du President Wilson, Paris 16th. Construction 1878-1894. Architect Leon Ginain (1825-1898). In order to give the City of Paris her art collections, the Duchess of Galliera built a museum in 1894, a pastiche of the Italian Renaissance. But for political reasons, it is the city of Genes (Italy) that houses the guilt and paintings while Paris remains the owner of this museum. / Bridgeman Images

ID: TEC4623978

The Musee Galliera, 14 avenue du President Wilson, Paris 16th. Construction 1878-1894. Architect Leon Ginain (1825-1898). In order to give the City of Paris her art collections, the Duchess of Galliera built a museum in 1894, a pastiche of the Italian Renaissance. But for political reasons, it is the city of Genes (Italy) that houses the guilt and paintings while Paris remains the owner of this museum.

Passy cemetery in Paris.
Passy cemetery in Paris.

TEC4623997: Passy cemetery in Paris. / Bridgeman Images

ID: TEC4623997

Passy cemetery in Paris.

The Palais de Tokyo has Paris from Avenue de New York, Paris 16th. Construction 1937, architects: Andre Aubert, Paul Viard, Jean Claude Dondel and Marcel Dastugue. Built for the 1937 World Exposition, it now houses in the east wing the Museum of Modern Art of the City of Paris. France, an immense allegory of Antoine Bourdelle, dominates the court in all its verticalite. Built in 1948 by the Free French Association.
The Palais de Tokyo has Paris from Avenue de New York, Paris 16th. Construction 1937, architects: Andre Aubert, Paul Viard, Jean Claude Dondel and Marcel Dastugue. Built for the 1937 World Exposition, it now houses in the east wing the Museum of Modern Art of the City of Paris. France, an immense allegory of Antoine Bourdelle, dominates the court in all its verticalite. Built in 1948 by the Free French Association.

TEC4624021: The Palais de Tokyo has Paris from Avenue de New York, Paris 16th. Construction 1937, architects: Andre Aubert, Paul Viard, Jean Claude Dondel and Marcel Dastugue. Built for the 1937 World Exposition, it now houses in the east wing the Museum of Modern Art of the City of Paris. France, an immense allegory of Antoine Bourdelle, dominates the court in all its verticalite. Built in 1948 by the Free French Association. / Bridgeman Images

ID: TEC4624021

The Palais de Tokyo has Paris from Avenue de New York, Paris 16th. Construction 1937, architects: Andre Aubert, Paul Viard, Jean Claude Dondel and Marcel Dastugue. Built for the 1937 World Exposition, it now houses in the east wing the Museum of Modern Art of the City of Paris. France, an immense allegory of Antoine Bourdelle, dominates the court in all its verticalite. Built in 1948 by the Free French Association.


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