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La Nouvelle Synagogue, 30 Oranienburger strasse, qaurtier Mitte in Berlin (Germany). Architects Eduard Knoblauch and Friedrich August Stuler, 1866, reconstruction Bernard Leisering, 1991. Photography 15/10/99.
La Nouvelle Synagogue, 30 Oranienburger strasse, qaurtier Mitte in Berlin (Germany). Architects Eduard Knoblauch and Friedrich August Stuler, 1866, reconstruction Bernard Leisering, 1991. Photography 15/10/99.

LBY4620646: La Nouvelle Synagogue, 30 Oranienburger strasse, qaurtier Mitte in Berlin (Germany). Architects Eduard Knoblauch and Friedrich August Stuler, 1866, reconstruction Bernard Leisering, 1991. Photography 15/10/99. / Bridgeman Images

ID: LBY4620646

La Nouvelle Synagogue, 30 Oranienburger strasse, qaurtier Mitte in Berlin (Germany). Architects Eduard Knoblauch and Friedrich August Stuler, 1866, reconstruction Bernard Leisering, 1991. Photography 15/10/99.

Einstein Cafe on Unter den Linden a Berlinae (Germany).
Einstein Cafe on Unter den Linden a Berlinae (Germany).

LBY4620680: Einstein Cafe on Unter den Linden a Berlinae (Germany). / Bridgeman Images

ID: LBY4620680

Einstein Cafe on Unter den Linden a Berlinae (Germany).

Nebula NGC 7635 in Cassiopee - North is at top. Seemingly adrift in a cosmic sea of stars and glowing gas, the delicate, floating apparition near the center (next to a blue tinted star) of this widefield view is cataloged as NGC 7635 - The Bubble Nebula. A mere 10 light - years wide, the tiny Bubble Nebula and the larger complex of interstellar gas and dust clouds are found about 11,000 light - years distant, straddling the boundary between the parental constellations Cepheus and Cassiopeia. Also included in the vista is open star cluster M52 (upper left), some 5,000 light - years away. The image spans about 2.7 degrees on the sky corresponding to a width of just over 500 light - years at the estimated distance of the Bubble Nebula. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory
Nebula NGC 7635 in Cassiopee - North is at top. Seemingly adrift in a cosmic sea of stars and glowing gas, the delicate, floating apparition near the center (next to a blue tinted star) of this widefield view is cataloged as NGC 7635 - The Bubble Nebula. A mere 10 light - years wide, the tiny Bubble Nebula and the larger complex of interstellar gas and dust clouds are found about 11,000 light - years distant, straddling the boundary between the parental constellations Cepheus and Cassiopeia. Also included in the vista is open star cluster M52 (upper left), some 5,000 light - years away. The image spans about 2.7 degrees on the sky corresponding to a width of just over 500 light - years at the estimated distance of the Bubble Nebula. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory

PIX4620650: Nebula NGC 7635 in Cassiopee - North is at top. Seemingly adrift in a cosmic sea of stars and glowing gas, the delicate, floating apparition near the center (next to a blue tinted star) of this widefield view is cataloged as NGC 7635 - The Bubble Nebula. A mere 10 light - years wide, the tiny Bubble Nebula and the larger complex of interstellar gas and dust clouds are found about 11,000 light - years distant, straddling the boundary between the parental constellations Cepheus and Cassiopeia. Also included in the vista is open star cluster M52 (upper left), some 5,000 light - years away. The image spans about 2.7 degrees on the sky corresponding to a width of just over 500 light - years at the estimated distance of the Bubble Nebula. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory / Bridgeman Images

ID: PIX4620650

Nebula NGC 7635 in Cassiopee - North is at top. Seemingly adrift in a cosmic sea of stars and glowing gas, the delicate, floating apparition near the center (next to a blue tinted star) of this widefield view is cataloged as NGC 7635 - The Bubble Nebula. A mere 10 light - years wide, the tiny Bubble Nebula and the larger complex of interstellar gas and dust clouds are found about 11,000 light - years distant, straddling the boundary between the parental constellations Cepheus and Cassiopeia. Also included in the vista is open star cluster M52 (upper left), some 5,000 light - years away. The image spans about 2.7 degrees on the sky corresponding to a width of just over 500 light - years at the estimated distance of the Bubble Nebula. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory

Nebula NGC 7635 in Cassiopee - This nebula is located about 7800 light years from Earth. A massive star, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522, 40 times more massive than our Sun. Image obtained by Isaac Newton 2.5m telescope from La Palma
Nebula NGC 7635 in Cassiopee - This nebula is located about 7800 light years from Earth. A massive star, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522, 40 times more massive than our Sun. Image obtained by Isaac Newton 2.5m telescope from La Palma

PIX4620665: Nebula NGC 7635 in Cassiopee - This nebula is located about 7800 light years from Earth. A massive star, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522, 40 times more massive than our Sun. Image obtained by Isaac Newton 2.5m telescope from La Palma / Bridgeman Images

ID: PIX4620665

Nebula NGC 7635 in Cassiopee - This nebula is located about 7800 light years from Earth. A massive star, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522, 40 times more massive than our Sun. Image obtained by Isaac Newton 2.5m telescope from La Palma

Nebula N119 in the Great Magellan Cloud - N119 is a “” H II region”” in the LMC
Nebula N119 in the Great Magellan Cloud - N119 is a “” H II region”” in the LMC

PIX4620774: Nebula N119 in the Great Magellan Cloud - N119 is a “” H II region”” in the LMC / Bridgeman Images

ID: PIX4620774

Nebula N119 in the Great Magellan Cloud - N119 is a “” H II region”” in the LMC

Nebula NGC 7635 in Cassiopee - The Bubble Nebula: This nebula is located about 8000 light years from Earth. A star 40 times more massive than our Sun, called Wolf-Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. Image obtained by the space telescope Hubble - The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8 000 light-years away - This complete view of the Bubble Nebula allows us to fully appreciate the almost perfectly symmetrical shell which gives the nebula its name. This shell is the result of a powerful flow of gas - known as a stellar wind - from the bright star visible just to the left of centre in this image. The star, SAO 20575, is between ten and twenty times the mass of the Sun and the pressure created by its stellar wind forces the surrounding interstellar material outwards into this bubble-like form - The giant molecular cloud that surrounds the star - glowing in the star's intense ultraviolet radiation - tries to stop the expansion of the bubble. However, although the sphere already measures around ten light-years in diameter, it is still growing, owing to the constant pressure of the stellar wind - currently at more than 100,000 kilometers per hour! - This stunning new image was observed by the NASA/ESA Hubble Space Telescope
Nebula NGC 7635 in Cassiopee - The Bubble Nebula: This nebula is located about 8000 light years from Earth. A star 40 times more massive than our Sun, called Wolf-Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. Image obtained by the space telescope Hubble - The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8 000 light-years away - This complete view of the Bubble Nebula allows us to fully appreciate the almost perfectly symmetrical shell which gives the nebula its name. This shell is the result of a powerful flow of gas - known as a stellar wind - from the bright star visible just to the left of centre in this image. The star, SAO 20575, is between ten and twenty times the mass of the Sun and the pressure created by its stellar wind forces the surrounding interstellar material outwards into this bubble-like form - The giant molecular cloud that surrounds the star - glowing in the star's intense ultraviolet radiation - tries to stop the expansion of the bubble. However, although the sphere already measures around ten light-years in diameter, it is still growing, owing to the constant pressure of the stellar wind - currently at more than 100,000 kilometers per hour! - This stunning new image was observed by the NASA/ESA Hubble Space Telescope

PIX4620728: Nebula NGC 7635 in Cassiopee - The Bubble Nebula: This nebula is located about 8000 light years from Earth. A star 40 times more massive than our Sun, called Wolf-Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. Image obtained by the space telescope Hubble - The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8 000 light-years away - This complete view of the Bubble Nebula allows us to fully appreciate the almost perfectly symmetrical shell which gives the nebula its name. This shell is the result of a powerful flow of gas - known as a stellar wind - from the bright star visible just to the left of centre in this image. The star, SAO 20575, is between ten and twenty times the mass of the Sun and the pressure created by its stellar wind forces the surrounding interstellar material outwards into this bubble-like form - The giant molecular cloud that surrounds the star - glowing in the star's intense ultraviolet radiation - tries to stop the expansion of the bubble. However, although the sphere already measures around ten light-years in diameter, it is still growing, owing to the constant pressure of the stellar wind - currently at more than 100,000 kilometers per hour! - This stunning new image was observed by the NASA/ESA Hubble Space Telescope / Bridgeman Images

ID: PIX4620728

Nebula NGC 7635 in Cassiopee - The Bubble Nebula: This nebula is located about 8000 light years from Earth. A star 40 times more massive than our Sun, called Wolf-Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. Image obtained by the space telescope Hubble - The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8 000 light-years away - This complete view of the Bubble Nebula allows us to fully appreciate the almost perfectly symmetrical shell which gives the nebula its name. This shell is the result of a powerful flow of gas - known as a stellar wind - from the bright star visible just to the left of centre in this image. The star, SAO 20575, is between ten and twenty times the mass of the Sun and the pressure created by its stellar wind forces the surrounding interstellar material outwards into this bubble-like form - The giant molecular cloud that surrounds the star - glowing in the star's intense ultraviolet radiation - tries to

Nebula NGC 346 in the Small Magellan Cloud - Nebula NGC 346 in the Small Magellanic Cloud - Photo of the nebula NGC 346, located about 210,000 years ago - light in the galaxy of the Little Magellan Cloud, obtained by the 2.2-metre MPG/ESO telescope. Nebula NGC 346 in the Small Magellanic Cloud, a nearby irregular galaxy, seen by the 2.2 - metre MPG/ESO telescope at the La Silla Observatory in Chile
Nebula NGC 346 in the Small Magellan Cloud - Nebula NGC 346 in the Small Magellanic Cloud - Photo of the nebula NGC 346, located about 210,000 years ago - light in the galaxy of the Little Magellan Cloud, obtained by the 2.2-metre MPG/ESO telescope. Nebula NGC 346 in the Small Magellanic Cloud, a nearby irregular galaxy, seen by the 2.2 - metre MPG/ESO telescope at the La Silla Observatory in Chile

PIX4620841: Nebula NGC 346 in the Small Magellan Cloud - Nebula NGC 346 in the Small Magellanic Cloud - Photo of the nebula NGC 346, located about 210,000 years ago - light in the galaxy of the Little Magellan Cloud, obtained by the 2.2-metre MPG/ESO telescope. Nebula NGC 346 in the Small Magellanic Cloud, a nearby irregular galaxy, seen by the 2.2 - metre MPG/ESO telescope at the La Silla Observatory in Chile / Bridgeman Images

ID: PIX4620841

Nebula NGC 346 in the Small Magellan Cloud - Nebula NGC 346 in the Small Magellanic Cloud - Photo of the nebula NGC 346, located about 210,000 years ago - light in the galaxy of the Little Magellan Cloud, obtained by the 2.2-metre MPG/ESO telescope. Nebula NGC 346 in the Small Magellanic Cloud, a nearby irregular galaxy, seen by the 2.2 - metre MPG/ESO telescope at the La Silla Observatory in Chile

The Duomo (Cathedrale) of Milan, Italy. Photograph 10/08/90.
The Duomo (Cathedrale) of Milan, Italy. Photograph 10/08/90.

LBY4620921: The Duomo (Cathedrale) of Milan, Italy. Photograph 10/08/90. / Bridgeman Images

ID: LBY4620921

The Duomo (Cathedrale) of Milan, Italy. Photograph 10/08/90.

N66 Nebula in the Little Magellan Cloud - Photo of the N66 nebula in the galaxy of the Small Magellan Cloud obtained by the Hubble space telescope. At the center of this nebula, a cluster of very young stars, NGC 346 in which some stars are only 5 million years old.
N66 Nebula in the Little Magellan Cloud - Photo of the N66 nebula in the galaxy of the Small Magellan Cloud obtained by the Hubble space telescope. At the center of this nebula, a cluster of very young stars, NGC 346 in which some stars are only 5 million years old.

PIX4620847: N66 Nebula in the Little Magellan Cloud - Photo of the N66 nebula in the galaxy of the Small Magellan Cloud obtained by the Hubble space telescope. At the center of this nebula, a cluster of very young stars, NGC 346 in which some stars are only 5 million years old. / Bridgeman Images

ID: PIX4620847

N66 Nebula in the Little Magellan Cloud - Photo of the N66 nebula in the galaxy of the Small Magellan Cloud obtained by the Hubble space telescope. At the center of this nebula, a cluster of very young stars, NGC 346 in which some stars are only 5 million years old.

Nebula N55 in the Great Magellan Cloud - Star forming region north of the Great Magellan Cloud. Image from the 1.2m Schmidt UK Telescope of Siding Spring
Nebula N55 in the Great Magellan Cloud - Star forming region north of the Great Magellan Cloud. Image from the 1.2m Schmidt UK Telescope of Siding Spring

PIX4620885: Nebula N55 in the Great Magellan Cloud - Star forming region north of the Great Magellan Cloud. Image from the 1.2m Schmidt UK Telescope of Siding Spring / Bridgeman Images

ID: PIX4620885

Nebula N55 in the Great Magellan Cloud - Star forming region north of the Great Magellan Cloud. Image from the 1.2m Schmidt UK Telescope of Siding Spring

Nebula N55 in the Great Magellan Cloud - Henize 55 (NGC 2014) is a star-forming region located north of the Great Magellan Cloud. Image obtained by Siding Spring's 3.9m telescope
Nebula N55 in the Great Magellan Cloud - Henize 55 (NGC 2014) is a star-forming region located north of the Great Magellan Cloud. Image obtained by Siding Spring's 3.9m telescope

PIX4620894: Nebula N55 in the Great Magellan Cloud - Henize 55 (NGC 2014) is a star-forming region located north of the Great Magellan Cloud. Image obtained by Siding Spring's 3.9m telescope / Bridgeman Images

ID: PIX4620894

Nebula N55 in the Great Magellan Cloud - Henize 55 (NGC 2014) is a star-forming region located north of the Great Magellan Cloud. Image obtained by Siding Spring's 3.9m telescope

On July 16, 1789, when King Louis XVI (1754-1793) en route to the town hall to receive the cocarde, 1907 (illustration)
On July 16, 1789, when King Louis XVI (1754-1793) en route to the town hall to receive the cocarde, 1907 (illustration)

JLJ4620907: On July 16, 1789, when King Louis XVI (1754-1793) en route to the town hall to receive the cocarde, 1907 (illustration), Vogel, Hermann (1856-1918) / Bridgeman Images

ID: JLJ4620907

On July 16, 1789, when King Louis XVI (1754-1793) en route to the town hall to receive the cocarde, 1907 (illustration)

Vogel, Hermann (1856-1918)

The Duomo di San Lorenzo of the Cathedral of Genes Duomo di San Lorenzo - Cathedrale de Genes - 1181
The Duomo di San Lorenzo of the Cathedral of Genes Duomo di San Lorenzo - Cathedrale de Genes - 1181

LBY4620931: The Duomo di San Lorenzo of the Cathedral of Genes Duomo di San Lorenzo - Cathedrale de Genes - 1181 / Bridgeman Images

ID: LBY4620931

The Duomo di San Lorenzo of the Cathedral of Genes Duomo di San Lorenzo - Cathedrale de Genes - 1181

La Nouvelle Synagogue, 30 Oranienburger strasse, qaurtier Mitte in Berlin (Germany). Architects Eduard Knoblauch and Friedrich August Stuler, 1866, reconstruction Bernard Leisering, 1991. Photography 15/10/99.
La Nouvelle Synagogue, 30 Oranienburger strasse, qaurtier Mitte in Berlin (Germany). Architects Eduard Knoblauch and Friedrich August Stuler, 1866, reconstruction Bernard Leisering, 1991. Photography 15/10/99.

LBY4620657: La Nouvelle Synagogue, 30 Oranienburger strasse, qaurtier Mitte in Berlin (Germany). Architects Eduard Knoblauch and Friedrich August Stuler, 1866, reconstruction Bernard Leisering, 1991. Photography 15/10/99. / Bridgeman Images

ID: LBY4620657

La Nouvelle Synagogue, 30 Oranienburger strasse, qaurtier Mitte in Berlin (Germany). Architects Eduard Knoblauch and Friedrich August Stuler, 1866, reconstruction Bernard Leisering, 1991. Photography 15/10/99.

Nebula NGC 7635 in Cassiopee - The Bubble Nebula (NGC 7635) in Cassiopeia - This nebula is located about 7100 years - light from Earth. A star 40 times more massive than our Sun, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. The Bubble Nebula in Cassiopeia is one of the most dramatic emission nebulae visible in the northern hemisphere. Lying at a distance of about 7,000 light - years away and spanning six light - years in diameter, NGC 7635 is quite bright with a magnitude of 7.0. The star in the middle of the bubble, BD+602522, is responsible for this stunning site, for this very hot star emits so much UV radiation that it is able to also heat and excite the surrounding dust and gas, thus emitting its own radiation. It is a Wolf - Rayet star, a very luminous star and also very short - lived. This Wolf - Rayet star is 40 times as massive than our sun
Nebula NGC 7635 in Cassiopee - The Bubble Nebula (NGC 7635) in Cassiopeia - This nebula is located about 7100 years - light from Earth. A star 40 times more massive than our Sun, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. The Bubble Nebula in Cassiopeia is one of the most dramatic emission nebulae visible in the northern hemisphere. Lying at a distance of about 7,000 light - years away and spanning six light - years in diameter, NGC 7635 is quite bright with a magnitude of 7.0. The star in the middle of the bubble, BD+602522, is responsible for this stunning site, for this very hot star emits so much UV radiation that it is able to also heat and excite the surrounding dust and gas, thus emitting its own radiation. It is a Wolf - Rayet star, a very luminous star and also very short - lived. This Wolf - Rayet star is 40 times as massive than our sun

PIX4620709: Nebula NGC 7635 in Cassiopee - The Bubble Nebula (NGC 7635) in Cassiopeia - This nebula is located about 7100 years - light from Earth. A star 40 times more massive than our Sun, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. The Bubble Nebula in Cassiopeia is one of the most dramatic emission nebulae visible in the northern hemisphere. Lying at a distance of about 7,000 light - years away and spanning six light - years in diameter, NGC 7635 is quite bright with a magnitude of 7.0. The star in the middle of the bubble, BD+602522, is responsible for this stunning site, for this very hot star emits so much UV radiation that it is able to also heat and excite the surrounding dust and gas, thus emitting its own radiation. It is a Wolf - Rayet star, a very luminous star and also very short - lived. This Wolf - Rayet star is 40 times as massive than our sun / Bridgeman Images

ID: PIX4620709

Nebula NGC 7635 in Cassiopee - The Bubble Nebula (NGC 7635) in Cassiopeia - This nebula is located about 7100 years - light from Earth. A star 40 times more massive than our Sun, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. The Bubble Nebula in Cassiopeia is one of the most dramatic emission nebulae visible in the northern hemisphere. Lying at a distance of about 7,000 light - years away and spanning six light - years in diameter, NGC 7635 is quite bright with a magnitude of 7.0. The star in the middle of the bubble, BD+602522, is responsible for this stunning site, for this very hot star emits so much UV radiation that it is able to also heat and excite the surrounding dust and gas, thus emitting its own radiation. It is a Wolf - Rayet star, a very luminous star and also very short - lived. This Wolf - Rayet star is 40 times as massive than our sun

Portrait of Philippe Coypel, brother of the artist Painting by Charles Antoine Coypel (1696-1752) 1732 Dim. 75x61 cm Paris, musee du Louvre
Portrait of Philippe Coypel, brother of the artist Painting by Charles Antoine Coypel (1696-1752) 1732 Dim. 75x61 cm Paris, musee du Louvre

LRI4620764: Portrait of Philippe Coypel, brother of the artist Painting by Charles Antoine Coypel (1696-1752) 1732 Dim. 75x61 cm Paris, musee du Louvre, Coypel, Antoine (1661-1722) / Bridgeman Images

ID: LRI4620764

Portrait of Philippe Coypel, brother of the artist Painting by Charles Antoine Coypel (1696-1752) 1732 Dim. 75x61 cm Paris, musee du Louvre

Coypel, Antoine (1661-1722)

The Dutch Nobles Walk on horseback. Painting by Albert (Aelbert or Aelbrecht) Cuyp (1620-1691) 17th century Sun. 119x152,5 cm Paris, musee du Louvre
The Dutch Nobles Walk on horseback. Painting by Albert (Aelbert or Aelbrecht) Cuyp (1620-1691) 17th century Sun. 119x152,5 cm Paris, musee du Louvre

LRI4620800: The Dutch Nobles Walk on horseback. Painting by Albert (Aelbert or Aelbrecht) Cuyp (1620-1691) 17th century Sun. 119x152,5 cm Paris, musee du Louvre, Cuyp, Aelbert (1620-91) / Bridgeman Images

ID: LRI4620800

The Dutch Nobles Walk on horseback. Painting by Albert (Aelbert or Aelbrecht) Cuyp (1620-1691) 17th century Sun. 119x152,5 cm Paris, musee du Louvre

Cuyp, Aelbert (1620-91)

The Victor Emmanuel II gallery in Milan, Italy. Architect Giuseppe Mengoni. Photography 10/08/90.
The Victor Emmanuel II gallery in Milan, Italy. Architect Giuseppe Mengoni. Photography 10/08/90.

LBY4620925: The Victor Emmanuel II gallery in Milan, Italy. Architect Giuseppe Mengoni. Photography 10/08/90. / Bridgeman Images

ID: LBY4620925

The Victor Emmanuel II gallery in Milan, Italy. Architect Giuseppe Mengoni. Photography 10/08/90.

The field concert Musicians on the grass, women are naked. Detail. Painting attributed to Tiziano Vecellio known as the Titian (1485-1576) or to Giorgio da Castelfranco called Giorgione (1476/1478-1510) Sun. 1,05 X 1.36 m Paris, Museum of the Louvre
The field concert Musicians on the grass, women are naked. Detail. Painting attributed to Tiziano Vecellio known as the Titian (1485-1576) or to Giorgio da Castelfranco called Giorgione (1476/1478-1510) Sun. 1,05 X 1.36 m Paris, Museum of the Louvre

LRI4621066: The field concert Musicians on the grass, women are naked. Detail. Painting attributed to Tiziano Vecellio known as the Titian (1485-1576) or to Giorgio da Castelfranco called Giorgione (1476/1478-1510) Sun. 1,05 X 1.36 m Paris, Museum of the Louvre, Titian (Tiziano Vecellio) (c.1488-1576) (attr. to) / Bridgeman Images

ID: LRI4621066

The field concert Musicians on the grass, women are naked. Detail. Painting attributed to Tiziano Vecellio known as the Titian (1485-1576) or to Giorgio da Castelfranco called Giorgione (1476/1478-1510) Sun. 1,05 X 1.36 m Paris, Museum of the Louvre

Titian (Tiziano Vecellio) (c.1488-1576) (attr. to)

St Bonaventure Enters the Franciscan Order (oil on canvas, 1628)
St Bonaventure Enters the Franciscan Order (oil on canvas, 1628)

LRI4621138: St Bonaventure Enters the Franciscan Order (oil on canvas, 1628), Herrera, Francisco (1576-1656) / Bridgeman Images

ID: LRI4621138

St Bonaventure Enters the Franciscan Order (oil on canvas, 1628)

Herrera, Francisco (1576-1656)

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

JLJ4621222: Pieright of the portal on the right of the western facade of the Basilica of Saint Denis, France (photo), French School / Bridgeman Images

ID: JLJ4621222

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

French School

Sixth Italian War (1521-1526): the fleet from Doria to Naples, Italy, 1909 (illustration)
Sixth Italian War (1521-1526): the fleet from Doria to Naples, Italy, 1909 (illustration)

JLJ4620994: Sixth Italian War (1521-1526): the fleet from Doria to Naples, Italy, 1909 (illustration), Robida, Albert (1848-1926) / Bridgeman Images

ID: JLJ4620994

Sixth Italian War (1521-1526): the fleet from Doria to Naples, Italy, 1909 (illustration)

Robida, Albert (1848-1926)

Nebuleuse Sh2 - 155 in Cephe
Nebuleuse Sh2 - 155 in Cephe

PIX4621081: Nebuleuse Sh2 - 155 in Cephe / Bridgeman Images

ID: PIX4621081

Nebuleuse Sh2 - 155 in Cephe

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)

JLJ4621202: Pieright of the right-hand portal of the western facade of the Basilica of Saint Denis, France (photo), French School / Bridgeman Images

ID: JLJ4621202

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

French School

Nebula Sharpless 2 - 1 (SH2 - 1) in Scorpio - Nebula Sharpless 2 - 1 (SH2 - 1) in Scorpio
Nebula Sharpless 2 - 1 (SH2 - 1) in Scorpio - Nebula Sharpless 2 - 1 (SH2 - 1) in Scorpio

PIX4620950: Nebula Sharpless 2 - 1 (SH2 - 1) in Scorpio - Nebula Sharpless 2 - 1 (SH2 - 1) in Scorpio / Bridgeman Images

ID: PIX4620950

Nebula Sharpless 2 - 1 (SH2 - 1) in Scorpio - Nebula Sharpless 2 - 1 (SH2 - 1) in Scorpio

Jean Ango's fleet blocked the Tagus River and threatened Lisbon in 1531, 1909 (illustration)
Jean Ango's fleet blocked the Tagus River and threatened Lisbon in 1531, 1909 (illustration)

JLJ4621026: Jean Ango's fleet blocked the Tagus River and threatened Lisbon in 1531, 1909 (illustration), Robida, Albert (1848-1926) / Bridgeman Images

ID: JLJ4621026

Jean Ango's fleet blocked the Tagus River and threatened Lisbon in 1531, 1909 (illustration)

Robida, Albert (1848-1926)

Nebula Sh2 - 142 in Cephee - Star formation region in Cephee and star clusters NGC 7380
Nebula Sh2 - 142 in Cephee - Star formation region in Cephee and star clusters NGC 7380

PIX4621042: Nebula Sh2 - 142 in Cephee - Star formation region in Cephee and star clusters NGC 7380 / Bridgeman Images

ID: PIX4621042

Nebula Sh2 - 142 in Cephee - Star formation region in Cephee and star clusters NGC 7380

Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star formation 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. Composite image in different wavelengths obtained by the Spitzer space telescope; in blue the visible light, in yellow and red the infrared light. 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. This colorful image is a large - scale composite mosaic assembled from data collected at a variety of different wavelengths. Views at visible wavelengths appear blue, near - infrared light is depicted as green, and mid - infrared data is portrayed as red. The result is a contrast between structures seen in visible light (blue) and those observed in the infrared (yellow and red). The image covers an area about two times that of a full moon. The red filaments stretching across the Spitzer image denote the presence of polycyclic aromatic hydrocarbons. These organic molecules, comprised of carbon and hydrogen, are excited by surrounding i
Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star formation 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. Composite image in different wavelengths obtained by the Spitzer space telescope; in blue the visible light, in yellow and red the infrared light. 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. This colorful image is a large - scale composite mosaic assembled from data collected at a variety of different wavelengths. Views at visible wavelengths appear blue, near - infrared light is depicted as green, and mid - infrared data is portrayed as red. The result is a contrast between structures seen in visible light (blue) and those observed in the infrared (yellow and red). The image covers an area about two times that of a full moon. The red filaments stretching across the Spitzer image denote the presence of polycyclic aromatic hydrocarbons. These organic molecules, comprised of carbon and hydrogen, are excited by surrounding i

PIX4621115: Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star formation 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. Composite image in different wavelengths obtained by the Spitzer space telescope; in blue the visible light, in yellow and red the infrared light. 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. This colorful image is a large - scale composite mosaic assembled from data collected at a variety of different wavelengths. Views at visible wavelengths appear blue, near - infrared light is depicted as green, and mid - infrared data is portrayed as red. The result is a contrast between structures seen in visible light (blue) and those observed in the infrared (yellow and red). The image covers an area about two times that of a full moon. The red filaments stretching across the Spitzer image denote the presence of polycyclic aromatic hydrocarbons. These organic molecules, comprised of carbon and hydrogen, are excited by surrounding i / Bridgeman Images

ID: PIX4621115

Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star formation 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. Composite image in different wavelengths obtained by the Spitzer space telescope; in blue the visible light, in yellow and red the infrared light. 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

Portrait of the Reepmaker family (oil on canvas, 1669)
Portrait of the Reepmaker family (oil on canvas, 1669)

LRI4621135: Portrait of the Reepmaker family (oil on canvas, 1669), Helst, Bartolomeus van der (1613-70) / Bridgeman Images

ID: LRI4621135

Portrait of the Reepmaker family (oil on canvas, 1669)

Helst, Bartolomeus van der (1613-70)

Sixth Italian War (1521-1526): women at the seat of Marseille in 1524, siege, 1909 (illustration)
Sixth Italian War (1521-1526): women at the seat of Marseille in 1524, siege, 1909 (illustration)

JLJ4621140: Sixth Italian War (1521-1526): women at the seat of Marseille in 1524, siege, 1909 (illustration), Robida, Albert (1848-1926) / Bridgeman Images

ID: JLJ4621140

Sixth Italian War (1521-1526): women at the seat of Marseille in 1524, siege, 1909 (illustration)

Robida, Albert (1848-1926)

Dark nebula and globular cluster NGC 4372 - Dark nebula and globular cluster NGC 4372 - HMSTG 436 is a molecular cloud visible near the globular cluster NGC 4372 (on the right, above the bright star Gamma Musca) in the southern constellation of the Fly. HMSTG 436 is a linear molecular cloud in the southern constellation Musca, the fly. It is easily found by targeting the globular cluster NGC 4372, visible at right, above the bright star gamma Musca
Dark nebula and globular cluster NGC 4372 - Dark nebula and globular cluster NGC 4372 - HMSTG 436 is a molecular cloud visible near the globular cluster NGC 4372 (on the right, above the bright star Gamma Musca) in the southern constellation of the Fly. HMSTG 436 is a linear molecular cloud in the southern constellation Musca, the fly. It is easily found by targeting the globular cluster NGC 4372, visible at right, above the bright star gamma Musca

PIX4621162: Dark nebula and globular cluster NGC 4372 - Dark nebula and globular cluster NGC 4372 - HMSTG 436 is a molecular cloud visible near the globular cluster NGC 4372 (on the right, above the bright star Gamma Musca) in the southern constellation of the Fly. HMSTG 436 is a linear molecular cloud in the southern constellation Musca, the fly. It is easily found by targeting the globular cluster NGC 4372, visible at right, above the bright star gamma Musca / Bridgeman Images

ID: PIX4621162

Dark nebula and globular cluster NGC 4372 - Dark nebula and globular cluster NGC 4372 - HMSTG 436 is a molecular cloud visible near the globular cluster NGC 4372 (on the right, above the bright star Gamma Musca) in the southern constellation of the Fly. HMSTG 436 is a linear molecular cloud in the southern constellation Musca, the fly. It is easily found by targeting the globular cluster NGC 4372, visible at right, above the bright star gamma Musca

Portrait of a member of the Belveze-Foulon family (Belveze Foulon). Painting by Jean-Auguste-Dominique Ingres (1780-1867) (Jean-Auguste-Dominique Ingres), 1805. Oil on canvas. Dim: 55x46cm. Montauban, Musee Ingres
Portrait of a member of the Belveze-Foulon family (Belveze Foulon). Painting by Jean-Auguste-Dominique Ingres (1780-1867) (Jean-Auguste-Dominique Ingres), 1805. Oil on canvas. Dim: 55x46cm. Montauban, Musee Ingres

LRI4621187: Portrait of a member of the Belveze-Foulon family (Belveze Foulon). Painting by Jean-Auguste-Dominique Ingres (1780-1867) (Jean-Auguste-Dominique Ingres), 1805. Oil on canvas. Dim: 55x46cm. Montauban, Musee Ingres, Ingres, Jean Auguste Dominique (1780-1867) / Bridgeman Images

ID: LRI4621187

Portrait of a member of the Belveze-Foulon family (Belveze Foulon). Painting by Jean-Auguste-Dominique Ingres (1780-1867) (Jean-Auguste-Dominique Ingres), 1805. Oil on canvas. Dim: 55x46cm. Montauban, Musee Ingres

Ingres, Jean Auguste Dominique (1780-1867)

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

JLJ4621224: Piedroit of the right-hand portal of the western facade of the Basilica of Saint Denis, France (photo), French School / Bridgeman Images

ID: JLJ4621224

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

French School

Nebulae B175 and VDB 152 in Cephee - Dark nebula B175 and reflection nebula VDB 152 - In the center of the image, 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). In the center of the image a large dust band, B175; above is the reflection nebula VDB 152 (or Ced 201). These objects are located in Cepheus constellation
Nebulae B175 and VDB 152 in Cephee - Dark nebula B175 and reflection nebula VDB 152 - In the center of the image, 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). In the center of the image a large dust band, B175; above is the reflection nebula VDB 152 (or Ced 201). These objects are located in Cepheus constellation

PIX4621239: Nebulae B175 and VDB 152 in Cephee - Dark nebula B175 and reflection nebula VDB 152 - In the center of the image, 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). In the center of the image a large dust band, B175; above is the reflection nebula VDB 152 (or Ced 201). These objects are located in Cepheus constellation / Bridgeman Images

ID: PIX4621239

Nebulae B175 and VDB 152 in Cephee - Dark nebula B175 and reflection nebula VDB 152 - In the center of the image, 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). In the center of the image a large dust band, B175; above is the reflection nebula VDB 152 (or Ced 201). These objects are located in Cepheus constellation

The turkish bath, detail (1862 - Oil on wood)
The turkish bath, detail (1862 - Oil on wood)

LRI4621246: The turkish bath, detail (1862 - Oil on wood), Ingres, Jean Auguste Dominique (1780-1867) / Bridgeman Images

ID: LRI4621246

The turkish bath, detail (1862 - Oil on wood)

Ingres, Jean Auguste Dominique (1780-1867)

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)

JLJ4621249: Pieright of the right-hand portal of the western facade of the Basilica of Saint Denis, France (photo), French School / Bridgeman Images

ID: JLJ4621249

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

French School


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