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The Virgin of Consolation or Chardonneret. 15th century (High relief ceramic)
The Virgin of Consolation or Chardonneret. 15th century (High relief ceramic)

LRI4691130: The Virgin of Consolation or Chardonneret. 15th century (High relief ceramic), Della Robbia, Andrea (1435-1525/28) / Bridgeman Images

The Virgin and Child. 15th centruy (High relief ceramic)
The Virgin and Child. 15th centruy (High relief ceramic)

LRI4691138: The Virgin and Child. 15th centruy (High relief ceramic), Della Robbia, Luca (1400-82) / Bridgeman Images

Mary annunciation. Oval painting on anonymous dorus background of the Russian school. Rome, Russicum (Russian College)
Mary annunciation. Oval painting on anonymous dorus background of the Russian school. Rome, Russicum (Russian College)

LRI4691222: Mary annunciation. Oval painting on anonymous dorus background of the Russian school. Rome, Russicum (Russian College), Russian School / Bridgeman Images

View of the chapel, 1429-1481
View of the chapel, 1429-1481

LRI4691034: View of the chapel, 1429-1481, Italian School, (15th century) / Bridgeman Images

The Nativity with Saint Francis of Assisi and Saint Anthony of Padua. Representation of the Holy Trinity. c.1485 (High relief ceramic)
The Nativity with Saint Francis of Assisi and Saint Anthony of Padua. Representation of the Holy Trinity. c.1485 (High relief ceramic)

LRI4691102: The Nativity with Saint Francis of Assisi and Saint Anthony of Padua. Representation of the Holy Trinity. c.1485 (High relief ceramic), Robbia, Giovanni della (1469-c.1530) / Bridgeman Images

Saint Placide, Benedictine Monk Wood Painting by Nicola Filotesio dit Cola del 'Amatrice (1489-1559) Sun. 113,5x71 cm Fara Sabina (Rieti), Abbey of Farfa, Italy
Saint Placide, Benedictine Monk Wood Painting by Nicola Filotesio dit Cola del 'Amatrice (1489-1559) Sun. 113,5x71 cm Fara Sabina (Rieti), Abbey of Farfa, Italy

LRI4691173: Saint Placide, Benedictine Monk Wood Painting by Nicola Filotesio dit Cola del 'Amatrice (1489-1559) Sun. 113,5x71 cm Fara Sabina (Rieti), Abbey of Farfa, Italy, Cola dell'Amatrice (Nicola di Filotesio) (1489-c.1550) / Bridgeman Images

Portrait of Constant Poppy (1841-1904), 1864 (painting)
Portrait of Constant Poppy (1841-1904), 1864 (painting)

JLJ4619312: Portrait of Constant Poppy (1841-1904), 1864 (painting), Blanc, Joseph Paul (1846-1904) / Bridgeman Images

On the way to the derby, 19th century (engraving)
On the way to the derby, 19th century (engraving)

JLJ4619345: On the way to the derby, 19th century (engraving), Unknown Artist, (19th century) / Bridgeman Images

The PPlace de l'Homme de fer in Strasbourg (Bas Rhin, Alsace).
The PPlace de l'Homme de fer in Strasbourg (Bas Rhin, Alsace).

LBY4619349: The PPlace de l'Homme de fer in Strasbourg (Bas Rhin, Alsace). / Bridgeman Images

The foyer of the Opera. A tutu dancer chatting with gentlemen who came to greet them or taking a few steps to dance, 19th century (engraving)
The foyer of the Opera. A tutu dancer chatting with gentlemen who came to greet them or taking a few steps to dance, 19th century (engraving)

JLJ4619377: The foyer of the Opera. A tutu dancer chatting with gentlemen who came to greet them or taking a few steps to dance, 19th century (engraving), French School, (19th century) / Bridgeman Images

Nebulae NGC 6334 and NGC 6357 in Scorpio - Nebulae NGC 6334 and NGC 6357 in Scorpius: These nebulae are located about 5500 light years from Earth - Located in the constellation of Scorpius, the Cat's Paw Nebula resemble a faint, luminous paw-print on the sky. Deep images reveal that the nebula is about a degree across in the sky. At a distance of about 5500 light-years away it is a truly vast structure spanning almost 100 light-years across. The sculpted gases of NGC 6334 are illuminated by the light of numerous powerful stars, some exceeding 10 solar masses. The two brilliant blue stars in the upper left are Lambda and Kappa Scorpii. Many of these luminous hot stars are surprisingly not visible because they lie within the dusty plane of our galaxy. At infrared wavelengths the numerous hot stars are revealed and the nature of this object as a region of massive star formation becomes clear. In the past decade water masers, molecular outflows, and x-ray sources have provided direct evidence of clusters of protostars within NGC 6334. The nebula was discovered by John Herschel in 1837, and the brief and uninformative description in his Cape Observations catalog is a testament to its faintness. The ruddy hue of this complex is the result of the absorption of blue light by the ubiquitous dust clouds along our line of sight in the plane of the Milky Way. The red, intricate bubble making up the left paw print is particularly striking and is most likely either a star expelling large amounts of matter at high speed as it nears the end of its life or the remnant of a recent supernova - Located near the famous “” Cat Paw”” nebula (NGC 6334), the Stellar Cluster Pismis 24 lies at the core of NGC 6357. Its stars include some of the most massive stellar behemoths known. One of the brightest stars in the cluster, Pismis 24-1, was thought possibly to be the most massive on record, approaching 300 solar masses, until it was discovered by the Hubble Telescope to b
Nebulae NGC 6334 and NGC 6357 in Scorpio - Nebulae NGC 6334 and NGC 6357 in Scorpius: These nebulae are located about 5500 light years from Earth - Located in the constellation of Scorpius, the Cat's Paw Nebula resemble a faint, luminous paw-print on the sky. Deep images reveal that the nebula is about a degree across in the sky. At a distance of about 5500 light-years away it is a truly vast structure spanning almost 100 light-years across. The sculpted gases of NGC 6334 are illuminated by the light of numerous powerful stars, some exceeding 10 solar masses. The two brilliant blue stars in the upper left are Lambda and Kappa Scorpii. Many of these luminous hot stars are surprisingly not visible because they lie within the dusty plane of our galaxy. At infrared wavelengths the numerous hot stars are revealed and the nature of this object as a region of massive star formation becomes clear. In the past decade water masers, molecular outflows, and x-ray sources have provided direct evidence of clusters of protostars within NGC 6334. The nebula was discovered by John Herschel in 1837, and the brief and uninformative description in his Cape Observations catalog is a testament to its faintness. The ruddy hue of this complex is the result of the absorption of blue light by the ubiquitous dust clouds along our line of sight in the plane of the Milky Way. The red, intricate bubble making up the left paw print is particularly striking and is most likely either a star expelling large amounts of matter at high speed as it nears the end of its life or the remnant of a recent supernova - Located near the famous “” Cat Paw”” nebula (NGC 6334), the Stellar Cluster Pismis 24 lies at the core of NGC 6357. Its stars include some of the most massive stellar behemoths known. One of the brightest stars in the cluster, Pismis 24-1, was thought possibly to be the most massive on record, approaching 300 solar masses, until it was discovered by the Hubble Telescope to b

PIX4619391: Nebulae NGC 6334 and NGC 6357 in Scorpio - Nebulae NGC 6334 and NGC 6357 in Scorpius: These nebulae are located about 5500 light years from Earth - Located in the constellation of Scorpius, the Cat's Paw Nebula resemble a faint, luminous paw-print on the sky. Deep images reveal that the nebula is about a degree across in the sky. At a distance of about 5500 light-years away it is a truly vast structure spanning almost 100 light-years across. The sculpted gases of NGC 6334 are illuminated by the light of numerous powerful stars, some exceeding 10 solar masses. The two brilliant blue stars in the upper left are Lambda and Kappa Scorpii. Many of these luminous hot stars are surprisingly not visible because they lie within the dusty plane of our galaxy. At infrared wavelengths the numerous hot stars are revealed and the nature of this object as a region of massive star formation becomes clear. In the past decade water masers, molecular outflows, and x-ray sources have provided direct evidence of clusters of protostars within NGC 6334. The nebula was discovered by John Herschel in 1837, and the brief and uninformative description in his Cape Observations catalog is a testament to its faintness. The ruddy hue of this complex is the result of the absorption of blue light by the ubiquitous dust clouds along our line of sight in the plane of the Milky Way. The red, intricate bubble making up the left paw print is particularly striking and is most likely either a star expelling large amounts of matter at high speed as it nears the end of its life or the remnant of a recent supernova - Located near the famous “” Cat Paw”” nebula (NGC 6334), the Stellar Cluster Pismis 24 lies at the core of NGC 6357. Its stars include some of the most massive stellar behemoths known. One of the brightest stars in the cluster, Pismis 24-1, was thought possibly to be the most massive on record, approaching 300 solar masses, until it was discovered by the Hubble Telescope to b / Bridgeman Images

Tram to Strasbourg (Bas Rhin, Alsace).
Tram to Strasbourg (Bas Rhin, Alsace).

LBY4619407: Tram to Strasbourg (Bas Rhin, Alsace). / Bridgeman Images

Shelf, balusters for Queen Marie Amelie's bedroom alcove, delivered 3/14/1839 to Trianon, 1839 (object)
Shelf, balusters for Queen Marie Amelie's bedroom alcove, delivered 3/14/1839 to Trianon, 1839 (object)

JLJ4619429: Shelf, balusters for Queen Marie Amelie's bedroom alcove, delivered 3/14/1839 to Trianon, 1839 (object), Jacob-Desmalter, Francois H. G. (1770-1841) (attr. to) / Bridgeman Images

View of the Bundestag in Berlin (Germany). Architect Paul Wallot (1841-1912). Photography 10/08/03.
View of the Bundestag in Berlin (Germany). Architect Paul Wallot (1841-1912). Photography 10/08/03.

TEC4619734: View of the Bundestag in Berlin (Germany). Architect Paul Wallot (1841-1912). Photography 10/08/03. / Bridgeman Images

Portico of the former Anhalter Bahnhof (station), Askanischer Platz, in the district of Kreutzberg in Berlinae (Germany). Architect Franz Schwechten, 1876-1880.
Portico of the former Anhalter Bahnhof (station), Askanischer Platz, in the district of Kreutzberg in Berlinae (Germany). Architect Franz Schwechten, 1876-1880.

TEC4619791: Portico of the former Anhalter Bahnhof (station), Askanischer Platz, in the district of Kreutzberg in Berlinae (Germany). Architect Franz Schwechten, 1876-1880. / Bridgeman Images

Nebula NGC 6559 in Sagittarius - NGC 6559 and IC 1274 - 75 in Sagittarius - Located in Sagittarius, this nebula is located at a distance of about 5000 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. This dusty region is probably associated with the brighter and better - known Lagoon and Trifid Nebulae which are nearby in the sky and part of the same molecular cloud. The soft red glow of fluorescent hydrogen is evidence that there are young hot stars associated with the dusty clouds. These bright stars also illuminate the tiny solid particles, producing blue reflection nebulae bordering some of the emission regions. The dust is also evident in silhouette, both as sinuous dark lanes winding through the luminous gas and as the dark patches obscuring the ancient, yellow stars that populate the central parts of the Milky Way
Nebula NGC 6559 in Sagittarius - NGC 6559 and IC 1274 - 75 in Sagittarius - Located in Sagittarius, this nebula is located at a distance of about 5000 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. This dusty region is probably associated with the brighter and better - known Lagoon and Trifid Nebulae which are nearby in the sky and part of the same molecular cloud. The soft red glow of fluorescent hydrogen is evidence that there are young hot stars associated with the dusty clouds. These bright stars also illuminate the tiny solid particles, producing blue reflection nebulae bordering some of the emission regions. The dust is also evident in silhouette, both as sinuous dark lanes winding through the luminous gas and as the dark patches obscuring the ancient, yellow stars that populate the central parts of the Milky Way

PIX4619800: Nebula NGC 6559 in Sagittarius - NGC 6559 and IC 1274 - 75 in Sagittarius - Located in Sagittarius, this nebula is located at a distance of about 5000 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. This dusty region is probably associated with the brighter and better - known Lagoon and Trifid Nebulae which are nearby in the sky and part of the same molecular cloud. The soft red glow of fluorescent hydrogen is evidence that there are young hot stars associated with the dusty clouds. These bright stars also illuminate the tiny solid particles, producing blue reflection nebulae bordering some of the emission regions. The dust is also evident in silhouette, both as sinuous dark lanes winding through the luminous gas and as the dark patches obscuring the ancient, yellow stars that populate the central parts of the Milky Way / Bridgeman Images

Vendee War: pacification of the Vendee, in 1796. Low relief in marble carved, 1800, 1796 (marble)
Vendee War: pacification of the Vendee, in 1796. Low relief in marble carved, 1800, 1796 (marble)

JLJ4619815: Vendee War: pacification of the Vendee, in 1796. Low relief in marble carved, 1800, 1796 (marble), Boizot, Louis Simon (1743-1809) / Bridgeman Images

Store des Westens (KaDeWe), Tauentzienstasse 21/24, Schoneberg district in Berlin (Germany). Construction 1906-1907, architect Johann Emil Schaudt (1871-1957).
Store des Westens (KaDeWe), Tauentzienstasse 21/24, Schoneberg district in Berlin (Germany). Construction 1906-1907, architect Johann Emil Schaudt (1871-1957).

TEC4619873: Store des Westens (KaDeWe), Tauentzienstasse 21/24, Schoneberg district in Berlin (Germany). Construction 1906-1907, architect Johann Emil Schaudt (1871-1957). / Bridgeman Images

The Swiss seize the wealth of Charles the Temeraire (1433-1477), 1905 (illustration)
The Swiss seize the wealth of Charles the Temeraire (1433-1477), 1905 (illustration)

JLJ4619851: The Swiss seize the wealth of Charles the Temeraire (1433-1477), 1905 (illustration), Job, pseudonym for Onfray de Breville, Jacques (1858-1931) / Bridgeman Images

Tram to Strasbourg (Bas Rhin, Alsace).
Tram to Strasbourg (Bas Rhin, Alsace).

LBY4619471: Tram to Strasbourg (Bas Rhin, Alsace). / Bridgeman Images

Bodes Museum on the island of Musees in Berlin (Germany). Fly boat. Photograph 10/08/03.
Bodes Museum on the island of Musees in Berlin (Germany). Fly boat. Photograph 10/08/03.

TEC4619958: Bodes Museum on the island of Musees in Berlin (Germany). Fly boat. Photograph 10/08/03. / Bridgeman Images

The Bodes Museum on the island of the Musees in Berlin (Germany).
The Bodes Museum on the island of the Musees in Berlin (Germany).

TEC4619957: The Bodes Museum on the island of the Musees in Berlin (Germany). / Bridgeman Images

Four musicians. Three violinists and one cellist, 19th century (poster)
Four musicians. Three violinists and one cellist, 19th century (poster)

LRI4619922: Four musicians. Three violinists and one cellist, 19th century (poster), Hohenstein, Adolfo (1854-1928) / Bridgeman Images

Trifide nebula (M20) in the constellation Sagittarius: View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 light years from Earth. Measuring some forty light years across, this nebula contains enough gas to make many thousands of suns. Trifid is located in Sagittarius constellation between 5000 and 10,000 light-years away
Trifide nebula (M20) in the constellation Sagittarius: View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 light years from Earth. Measuring some forty light years across, this nebula contains enough gas to make many thousands of suns. Trifid is located in Sagittarius constellation between 5000 and 10,000 light-years away

PIX4619532: Trifide nebula (M20) in the constellation Sagittarius: View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 light years from Earth. Measuring some forty light years across, this nebula contains enough gas to make many thousands of suns. Trifid is located in Sagittarius constellation between 5000 and 10,000 light-years away / Bridgeman Images

Tacheless in the district of Kreutzbergæa Berlin (Germany).
Tacheless in the district of Kreutzbergæa Berlin (Germany).

TEC4619997: Tacheless in the district of Kreutzbergæa Berlin (Germany). / Bridgeman Images

France, Paris under the occupation June 1940: exodus of the population Gate d'Orleans (refugees leave Paris) (photo)
France, Paris under the occupation June 1940: exodus of the population Gate d'Orleans (refugees leave Paris) (photo)

JLJ4617826: France, Paris under the occupation June 1940: exodus of the population Gate d'Orleans (refugees leave Paris) (photo), Unknown photographer, (20th century) / Bridgeman Images

Paul Emile Victor (B/W photo, 1987)
Paul Emile Victor (B/W photo, 1987)

PEV6150461: Paul Emile Victor (B/W photo, 1987) / Bridgeman Images

Portrait of Sir Christopher Benson, seated, 1997-98 (oil on canvas)
Portrait of Sir Christopher Benson, seated, 1997-98 (oil on canvas)

CH6150698: Portrait of Sir Christopher Benson, seated, 1997-98 (oil on canvas), Noakes, Michael (1933-2018) / Bridgeman Images

Portrait of Lord Aldington, seated wearing a dark suit, 1984 (oil on canvas)
Portrait of Lord Aldington, seated wearing a dark suit, 1984 (oil on canvas)

CH6150709: Portrait of Lord Aldington, seated wearing a dark suit, 1984 (oil on canvas), Noakes, Michael (1933-2018) / Bridgeman Images

Portrait of Henry Lambert, seated, 1993 (oil on canvas)
Portrait of Henry Lambert, seated, 1993 (oil on canvas)

CH6150705: Portrait of Henry Lambert, seated, 1993 (oil on canvas), Noakes, Michael (1933-2018) / Bridgeman Images

Egyptian Museum, Turin, Italy, 2020 (photo)
Egyptian Museum, Turin, Italy, 2020 (photo)

BSI6302393: Egyptian Museum, Turin, Italy, 2020 (photo), Balossini, Camillo / Bridgeman Images

Mountain farm, 1921
Mountain farm, 1921

OVR6302432: Mountain farm, 1921, Peterssen, Hjalmer Eilif Emanuel (1852-1928) / Bridgeman Images

Piazza San Carlo, Turin, Italy, 2020 (photo)
Piazza San Carlo, Turin, Italy, 2020 (photo)

BSI6302206: Piazza San Carlo, Turin, Italy, 2020 (photo), Balossini, Camillo / Bridgeman Images

Castello del Valentino, Turin, Italy, 2020 (photo)
Castello del Valentino, Turin, Italy, 2020 (photo)

BSI6302221: Castello del Valentino, Turin, Italy, 2020 (photo), Balossini, Camillo / Bridgeman Images

Castello del Valentino, Turin, Italy, 2020 (photo)
Castello del Valentino, Turin, Italy, 2020 (photo)

BSI6302236: Castello del Valentino, Turin, Italy, 2020 (photo), Balossini, Camillo / Bridgeman Images

Piazza Castello, Monument to Emanuele Filiberto Duca d'Aosta, Turin, Italy, 2020 (photo)
Piazza Castello, Monument to Emanuele Filiberto Duca d'Aosta, Turin, Italy, 2020 (photo)

BSI6302259: Piazza Castello, Monument to Emanuele Filiberto Duca d'Aosta, Turin, Italy, 2020 (photo), Balossini, Camillo / Bridgeman Images


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