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6600 Search Results for carving

Titian monument
Titian monument

SLR3827871: Titian monument / Bridgeman Images

Titian monument
Titian monument

SLR3827872: Titian monument / Bridgeman Images

Titian monument
Titian monument

SLR3827865: Titian monument / Bridgeman Images

statue of King Khasekhemwy
statue of King Khasekhemwy

SVA660280: statue of King Khasekhemwy, Egyptian School / Bridgeman Images

The Omega nebula (M17) seen in infrared - M17 nebula in infrared - The Omega nebula (M17) seen in infrared by the Spitzer space telescope. M17 is a star-forming region about 6000 light years ago in the constellation Sagittarius. In the center of the nebula is a group of massive stars. The dust appears in red, the hot gas in green, the regions or this gas and the dust mixes in white. Nasa's Spitzer Space Telescope has captured an infrared view of the star - making cloud called M17, or the Swan nebula. The cloud, located about 6,000 light - years away in the constellation Sagittarius, is dominated by a central group of massive stars - - the most massive stars in the region. These central stars give off intense flows of expanding gas, which rush like rivers against dense piles of material, carving out the deep pocket at center of the picture. Winds from the region's other massive stars push back against these oncoming rivers, creating bow shocks like those that pile up in front of speeding boats. Three of these bow shocks are nestled in the upper left side of the central cavity, but are difficult to spot in this view. They are composed of compressed gas in addition to dust that glows at infrared wavelengths Spitzer can see. The smiley - shaped bow shocks curve away from the stellar winds of the central massive stars. This picture was taken with Spitzer's infrared array camera. It is a four - color composite, in which light with a wavelength of 3.6 microns is blue; 4.5 - micron light is green; 5.8 - micron light is orange; and 8 - micron light is red. Dust is red, hot gas is green and white is where gas and dust intermingle. Foreground and background stars appear scattered through the image
The Omega nebula (M17) seen in infrared - M17 nebula in infrared - The Omega nebula (M17) seen in infrared by the Spitzer space telescope. M17 is a star-forming region about 6000 light years ago in the constellation Sagittarius. In the center of the nebula is a group of massive stars. The dust appears in red, the hot gas in green, the regions or this gas and the dust mixes in white. Nasa's Spitzer Space Telescope has captured an infrared view of the star - making cloud called M17, or the Swan nebula. The cloud, located about 6,000 light - years away in the constellation Sagittarius, is dominated by a central group of massive stars - - the most massive stars in the region. These central stars give off intense flows of expanding gas, which rush like rivers against dense piles of material, carving out the deep pocket at center of the picture. Winds from the region's other massive stars push back against these oncoming rivers, creating bow shocks like those that pile up in front of speeding boats. Three of these bow shocks are nestled in the upper left side of the central cavity, but are difficult to spot in this view. They are composed of compressed gas in addition to dust that glows at infrared wavelengths Spitzer can see. The smiley - shaped bow shocks curve away from the stellar winds of the central massive stars. This picture was taken with Spitzer's infrared array camera. It is a four - color composite, in which light with a wavelength of 3.6 microns is blue; 4.5 - micron light is green; 5.8 - micron light is orange; and 8 - micron light is red. Dust is red, hot gas is green and white is where gas and dust intermingle. Foreground and background stars appear scattered through the image

PIX4620190: The Omega nebula (M17) seen in infrared - M17 nebula in infrared - The Omega nebula (M17) seen in infrared by the Spitzer space telescope. M17 is a star-forming region about 6000 light years ago in the constellation Sagittarius. In the center of the nebula is a group of massive stars. The dust appears in red, the hot gas in green, the regions or this gas and the dust mixes in white. Nasa's Spitzer Space Telescope has captured an infrared view of the star - making cloud called M17, or the Swan nebula. The cloud, located about 6,000 light - years away in the constellation Sagittarius, is dominated by a central group of massive stars - - the most massive stars in the region. These central stars give off intense flows of expanding gas, which rush like rivers against dense piles of material, carving out the deep pocket at center of the picture. Winds from the region's other massive stars push back against these oncoming rivers, creating bow shocks like those that pile up in front of speeding boats. Three of these bow shocks are nestled in the upper left side of the central cavity, but are difficult to spot in this view. They are composed of compressed gas in addition to dust that glows at infrared wavelengths Spitzer can see. The smiley - shaped bow shocks curve away from the stellar winds of the central massive stars. This picture was taken with Spitzer's infrared array camera. It is a four - color composite, in which light with a wavelength of 3.6 microns is blue; 4.5 - micron light is green; 5.8 - micron light is orange; and 8 - micron light is red. Dust is red, hot gas is green and white is where gas and dust intermingle. Foreground and background stars appear scattered through the image / Bridgeman Images

An Unknown Young Painter aged 18
An Unknown Young Painter aged 18

USB1155860: An Unknown Young Painter aged 18, Italian School, (16th century) / Bridgeman Images

Titian monument
Titian monument

SLR3827869: Titian monument / Bridgeman Images

Model 1896 Mauser 7 mm bolt action rifle used by the Boers (rifle, bolt action, Mauser, 7 mm M1896)
Model 1896 Mauser 7 mm bolt action rifle used by the Boers (rifle, bolt action, Mauser, 7 mm M1896)

NAM5930074: Model 1896 Mauser 7 mm bolt action rifle used by the Boers (rifle, bolt action, Mauser, 7 mm M1896), English School, (19th century) / Bridgeman Images

Nordic bronze age: hunters, rock carvings in Tanum, Sweden, 1800-500 BC
Nordic bronze age: hunters, rock carvings in Tanum, Sweden, 1800-500 BC

LRI4641047: Nordic bronze age: hunters, rock carvings in Tanum, Sweden, 1800-500 BC, Prehistoric / Bridgeman Images

Nordic bronze age: couple embracing, rock carvings in Tanum, Sweden, 1800-500 BC
Nordic bronze age: couple embracing, rock carvings in Tanum, Sweden, 1800-500 BC

LRI4641049: Nordic bronze age: couple embracing, rock carvings in Tanum, Sweden, 1800-500 BC, Prehistoric / Bridgeman Images

White and Steel Polars, 1945 (painted wood, steel, iron, and plexiglas)
White and Steel Polars, 1945 (painted wood, steel, iron, and plexiglas)

CVL500344: White and Steel Polars, 1945 (painted wood, steel, iron, and plexiglas) , Roszak, Theodore (1907-81) / Bridgeman Images

Mauser 7 mm Cavalry Carbine used by Boer Commandos, 1899
Mauser 7 mm Cavalry Carbine used by Boer Commandos, 1899

NAM5925756: Mauser 7 mm Cavalry Carbine used by Boer Commandos, 1899, German School, (19th century) / Bridgeman Images

February (Febbraio), by Benedetto da Milano upon drawing by Bramantino, c. 1503-1508, 16th century (tapestry)
February (Febbraio), by Benedetto da Milano upon drawing by Bramantino, c. 1503-1508, 16th century (tapestry)

MEP1266874: February (Febbraio), by Benedetto da Milano upon drawing by Bramantino, c. 1503-1508, 16th century (tapestry), Milano, Benedetto da (fl.1504-09) / Bridgeman Images

Mauser 7 mm Cavalry Carbine used by Boer Commandos, 1899
Mauser 7 mm Cavalry Carbine used by Boer Commandos, 1899

NAM5925754: Mauser 7 mm Cavalry Carbine used by Boer Commandos, 1899, German School, (19th century) / Bridgeman Images

Mauser 7 mm Cavalry Carbine used by Boer Commandos, 1899
Mauser 7 mm Cavalry Carbine used by Boer Commandos, 1899

NAM5925753: Mauser 7 mm Cavalry Carbine used by Boer Commandos, 1899, German School, (19th century) / Bridgeman Images

Mauser 7 mm Cavalry Carbine used by Boer Commandos, 1899
Mauser 7 mm Cavalry Carbine used by Boer Commandos, 1899

NAM5925752: Mauser 7 mm Cavalry Carbine used by Boer Commandos, 1899, German School, (19th century) / Bridgeman Images

Japan: Two women on a veranda, painted by Suzuki Harunobu (1724-1770), c. 1750.
Japan: Two women on a veranda, painted by Suzuki Harunobu (1724-1770), c. 1750.

PFH1170071: Japan: Two women on a veranda, painted by Suzuki Harunobu (1724-1770), c. 1750., Harunobu, Suzuki (1725-70) / Bridgeman Images

Mauser 7 mm Cavalry Carbine used by Boer Commandos, 1899
Mauser 7 mm Cavalry Carbine used by Boer Commandos, 1899

NAM5925755: Mauser 7 mm Cavalry Carbine used by Boer Commandos, 1899, German School, (19th century) / Bridgeman Images

Sheikh el
Sheikh el

SVA660242: Sheikh el, Egyptian School / Bridgeman Images

Julius Caesar, c.1455-1460 (marble with traces of bole (red clay) and limestone with traces of polychromy)
Julius Caesar, c.1455-1460 (marble with traces of bole (red clay) and limestone with traces of polychromy)

XCL500383: Julius Caesar, c.1455-1460 (marble with traces of bole (red clay) and limestone with traces of polychromy) , Mino da Fiesole (1430-1484) / Bridgeman Images

Siege of Leningrad
Siege of Leningrad

BOF6284899: Siege of Leningrad / Bridgeman Images

Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavities, and some can be seen as pink dots at the tips of the elephant - trunk - like pillars. The white knotty areas are where the youngest stars are forming. Red shows heated dust that pervades the region's cavities, while green highlights dense clouds. W5 spans an area of sky equivalent to four full moons and is about 6,500 light - years away in the constellation Cassiopeia. The Spitzer picture was taken over a period of 24 hours. Like other massive star - forming regions, such as Orion and Carina, W5 contains large cavities that were carved out by radiation and winds from the region's most massive stars. According to the theory of triggered star - formation, the carving out of these cavities pushes gas together, causing it to ignite into successive generations of new stars. This image contains some of the best evidence yet for the triggered star - formation theory. Scientists analyzing the photo have been able to sho
Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavities, and some can be seen as pink dots at the tips of the elephant - trunk - like pillars. The white knotty areas are where the youngest stars are forming. Red shows heated dust that pervades the region's cavities, while green highlights dense clouds. W5 spans an area of sky equivalent to four full moons and is about 6,500 light - years away in the constellation Cassiopeia. The Spitzer picture was taken over a period of 24 hours. Like other massive star - forming regions, such as Orion and Carina, W5 contains large cavities that were carved out by radiation and winds from the region's most massive stars. According to the theory of triggered star - formation, the carving out of these cavities pushes gas together, causing it to ignite into successive generations of new stars. This image contains some of the best evidence yet for the triggered star - formation theory. Scientists analyzing the photo have been able to sho

PIX4621152: Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavities, and some can be seen as pink dots at the tips of the elephant - trunk - like pillars. The white knotty areas are where the youngest stars are forming. Red shows heated dust that pervades the region's cavities, while green highlights dense clouds. W5 spans an area of sky equivalent to four full moons and is about 6,500 light - years away in the constellation Cassiopeia. The Spitzer picture was taken over a period of 24 hours. Like other massive star - forming regions, such as Orion and Carina, W5 contains large cavities that were carved out by radiation and winds from the region's most massive stars. According to the theory of triggered star - formation, the carving out of these cavities pushes gas together, causing it to ignite into successive generations of new stars. This image contains some of the best evidence yet for the triggered star - formation theory. Scientists analyzing the photo have been able to sho / Bridgeman Images

islamic art-panel-wood-inv.n.3391-purchased Ilyas Khatun-Fatimid 11th century-IM-11090-019
islamic art-panel-wood-inv.n.3391-purchased Ilyas Khatun-Fatimid 11th century-IM-11090-019

VIS693549: islamic art-panel-wood-inv.n.3391-purchased Ilyas Khatun-Fatimid 11th century-IM-11090-019 / Bridgeman Images

Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavities, and some can be seen as pink dots at the tips of the elephant - trunk - like pillars. The white knotty areas are where the youngest stars are forming. Red shows heated dust that pervades the region's cavities, while green highlights dense clouds. W5 spans an area of sky equivalent to four full moons and is about 6,500 light - years away in the constellation Cassiopeia. The Spitzer picture was taken over a period of 24 hours. Like other massive star - forming regions, such as Orion and Carina, W5 contains large cavities that were carved out by radiation and winds from the region's most massive stars. According to the theory of triggered star - formation, the carving out of these cavities pushes gas together, causing it to ignite into successive generations of new stars. This image contains some of the best evidence yet for the triggered star - formation theory. Scientists analyzing the photo have been able to sho
Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavities, and some can be seen as pink dots at the tips of the elephant - trunk - like pillars. The white knotty areas are where the youngest stars are forming. Red shows heated dust that pervades the region's cavities, while green highlights dense clouds. W5 spans an area of sky equivalent to four full moons and is about 6,500 light - years away in the constellation Cassiopeia. The Spitzer picture was taken over a period of 24 hours. Like other massive star - forming regions, such as Orion and Carina, W5 contains large cavities that were carved out by radiation and winds from the region's most massive stars. According to the theory of triggered star - formation, the carving out of these cavities pushes gas together, causing it to ignite into successive generations of new stars. This image contains some of the best evidence yet for the triggered star - formation theory. Scientists analyzing the photo have been able to sho

PIX4621160: Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavities, and some can be seen as pink dots at the tips of the elephant - trunk - like pillars. The white knotty areas are where the youngest stars are forming. Red shows heated dust that pervades the region's cavities, while green highlights dense clouds. W5 spans an area of sky equivalent to four full moons and is about 6,500 light - years away in the constellation Cassiopeia. The Spitzer picture was taken over a period of 24 hours. Like other massive star - forming regions, such as Orion and Carina, W5 contains large cavities that were carved out by radiation and winds from the region's most massive stars. According to the theory of triggered star - formation, the carving out of these cavities pushes gas together, causing it to ignite into successive generations of new stars. This image contains some of the best evidence yet for the triggered star - formation theory. Scientists analyzing the photo have been able to sho / Bridgeman Images

Woodcarving (wood)
Woodcarving (wood)

HGP362287: Woodcarving (wood), Gibbons, Grinling (1648-1721) / Bridgeman Images

islamic art-panel-wood-inv.n.3391-purchased Ilyas Khatun-Fatimid 11th century-IM-11090-017
islamic art-panel-wood-inv.n.3391-purchased Ilyas Khatun-Fatimid 11th century-IM-11090-017

VIS693576: islamic art-panel-wood-inv.n.3391-purchased Ilyas Khatun-Fatimid 11th century-IM-11090-017 / Bridgeman Images

May 05, 1953 - Student to receive Queen's Scout badge - and will help in the Royal kitchens.: Eleven boys from the Westminster Technical College, Vincent Square have been chosen to help in the Royal Kitchens when the Queen's Coronation guests arrive. They are receiving special instructions for the job - and the boys were chosen instead of girl students - as it is considered that they could stand the grest strain easier than the girls. Among them is Sixteen year old First year boy Peter Wells who belongs to the 35th. Westminster Sea Scout Troop.Peter will be going to the Mansion House soon to receive his certificate for the Queen's Scout badge
May 05, 1953 - Student to receive Queen's Scout badge - and will help in the Royal kitchens.: Eleven boys from the Westminster Technical College, Vincent Square have been chosen to help in the Royal Kitchens when the Queen's Coronation guests arrive. They are receiving special instructions for the job - and the boys were chosen instead of girl students - as it is considered that they could stand the grest strain easier than the girls. Among them is Sixteen year old First year boy Peter Wells who belongs to the 35th. Westminster Sea Scout Troop.Peter will be going to the Mansion House soon to receive his certificate for the Queen's Scout badge

ZUM4841289: May 05, 1953 - Student to receive Queen's Scout badge - and will help in the Royal kitchens.: Eleven boys from the Westminster Technical College, Vincent Square have been chosen to help in the Royal Kitchens when the Queen's Coronation guests arrive. They are receiving special instructions for the job - and the boys were chosen instead of girl students - as it is considered that they could stand the grest strain easier than the girls. Among them is Sixteen year old First year boy Peter Wells who belongs to the 35th. Westminster Sea Scout Troop.Peter will be going to the Mansion House soon to receive his certificate for the Queen's Scout badge / Bridgeman Images

Sheikh el
Sheikh el

SVA660241: Sheikh el, Egyptian School / Bridgeman Images

May 05, 1953 - Student To Receive Queen's Scout Badge - And Will Help In The Royal Kitchens; Eleven boys from the Westmineter Technical College, Vincent Square have been chosen to help in the Royal Kitchens when the Queen; s Coronation guests arrive. They are receiving special instructions for the job - and the boys were chosen instead of girl students - as it is considered that they could stand the great strain easier than the girls. Among them is Sixteen year old First Year boy Peter Wells who belongs to the 35th. Westminster Sea Scout Troop. Peter will be going to the Mansion House soon to receive his certificate for the Queen's Scout badge
May 05, 1953 - Student To Receive Queen's Scout Badge - And Will Help In The Royal Kitchens; Eleven boys from the Westmineter Technical College, Vincent Square have been chosen to help in the Royal Kitchens when the Queen; s Coronation guests arrive. They are receiving special instructions for the job - and the boys were chosen instead of girl students - as it is considered that they could stand the great strain easier than the girls. Among them is Sixteen year old First Year boy Peter Wells who belongs to the 35th. Westminster Sea Scout Troop. Peter will be going to the Mansion House soon to receive his certificate for the Queen's Scout badge

ZUM4841791: May 05, 1953 - Student To Receive Queen's Scout Badge - And Will Help In The Royal Kitchens; Eleven boys from the Westmineter Technical College, Vincent Square have been chosen to help in the Royal Kitchens when the Queen; s Coronation guests arrive. They are receiving special instructions for the job - and the boys were chosen instead of girl students - as it is considered that they could stand the great strain easier than the girls. Among them is Sixteen year old First Year boy Peter Wells who belongs to the 35th. Westminster Sea Scout Troop. Peter will be going to the Mansion House soon to receive his certificate for the Queen's Scout badge / Bridgeman Images

Japan: Nishiki-e woodblock print of the Imperial Diet Building in Tokyo, May 1895.
Japan: Nishiki-e woodblock print of the Imperial Diet Building in Tokyo, May 1895.

PFH1170070: Japan: Nishiki-e woodblock print of the Imperial Diet Building in Tokyo, May 1895. / Bridgeman Images

Nordic bronze age: boats and sledges, rock carvings in Tanum, Sweden, 1800-500 BC
Nordic bronze age: boats and sledges, rock carvings in Tanum, Sweden, 1800-500 BC

LRI4641061: Nordic bronze age: boats and sledges, rock carvings in Tanum, Sweden, 1800-500 BC, Prehistoric / Bridgeman Images

Black king, chess piece, India, 1820 circa (ivory)
Black king, chess piece, India, 1820 circa (ivory)

NAM5924011: Black king, chess piece, India, 1820 circa (ivory), Indian School, (19th century) / Bridgeman Images

Mauser 7 mm bolt action sporting rifle, c.1900 (rifle, bolt action, sporting, Mauser, 7 mm)
Mauser 7 mm bolt action sporting rifle, c.1900 (rifle, bolt action, sporting, Mauser, 7 mm)

NAM5930078: Mauser 7 mm bolt action sporting rifle, c.1900 (rifle, bolt action, sporting, Mauser, 7 mm), German School, (19th century) / Bridgeman Images

Mauser 7 mm bolt action sporting rifle, c.1900 (rifle, bolt action, sporting, Mauser, 7 mm)
Mauser 7 mm bolt action sporting rifle, c.1900 (rifle, bolt action, sporting, Mauser, 7 mm)

NAM5930077: Mauser 7 mm bolt action sporting rifle, c.1900 (rifle, bolt action, sporting, Mauser, 7 mm), German School, (19th century) / Bridgeman Images

Armorial Shield Supported by Angels, made in Beauvais, late 15th to early 16th century (painted & gilded oak)
Armorial Shield Supported by Angels, made in Beauvais, late 15th to early 16th century (painted & gilded oak)

PHL434203: Armorial Shield Supported by Angels, made in Beauvais, late 15th to early 16th century (painted & gilded oak) , French School / Bridgeman Images

Black king, chess piece, India, 1820 circa (ivory)
Black king, chess piece, India, 1820 circa (ivory)

NAM5924014: Black king, chess piece, India, 1820 circa (ivory), Behr, Carel Jacobus (1812-95) / Bridgeman Images


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