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Jean Sylvain Bailly, Mayor of Paris, French astronomer, mathematician, freemason and revolutionary, 1736-1793. In costume of depute in the States-General, 1789. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.
Jean Sylvain Bailly, Mayor of Paris, French astronomer, mathematician, freemason and revolutionary, 1736-1793. In costume of depute in the States-General, 1789. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.

FLO4572478: Jean Sylvain Bailly, Mayor of Paris, French astronomer, mathematician, freemason and revolutionary, 1736-1793. In costume of depute in the States-General, 1789. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852. / Bridgeman Images

ID: FLO4572478

Jean Sylvain Bailly, Mayor of Paris, French astronomer, mathematician, freemason and revolutionary, 1736-1793. In costume of depute in the States-General, 1789. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.

Jean Marie Roland, Viscount de la Platriere, Girondist and revolutionary 1752-1793. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.
Jean Marie Roland, Viscount de la Platriere, Girondist and revolutionary 1752-1793. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.

FLO4572486: Jean Marie Roland, Viscount de la Platriere, Girondist and revolutionary 1752-1793. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852. / Bridgeman Images

ID: FLO4572486

Jean Marie Roland, Viscount de la Platriere, Girondist and revolutionary 1752-1793. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.

The smallest stars - Artist's view - The smallest stars. Artwork - Comparison to the scale of the smallest stars with Jupiter and the Sun. From left to right: Jupiter, a brown dwarf (same size as Jupiter but 50 times more massive), dwarf L (younger brown dwarf), red dwarf, Sun. From left to right: Jupiter (a failed star), a brown dwarf (same size as Jupiter but 50 times more massive), a “” L”” dwarf (brown dwarf younger), a red dwarf and the sun for comparison
The smallest stars - Artist's view - The smallest stars. Artwork - Comparison to the scale of the smallest stars with Jupiter and the Sun. From left to right: Jupiter, a brown dwarf (same size as Jupiter but 50 times more massive), dwarf L (younger brown dwarf), red dwarf, Sun. From left to right: Jupiter (a failed star), a brown dwarf (same size as Jupiter but 50 times more massive), a “” L”” dwarf (brown dwarf younger), a red dwarf and the sun for comparison

PIX4572490: The smallest stars - Artist's view - The smallest stars. Artwork - Comparison to the scale of the smallest stars with Jupiter and the Sun. From left to right: Jupiter, a brown dwarf (same size as Jupiter but 50 times more massive), dwarf L (younger brown dwarf), red dwarf, Sun. From left to right: Jupiter (a failed star), a brown dwarf (same size as Jupiter but 50 times more massive), a “” L”” dwarf (brown dwarf younger), a red dwarf and the sun for comparison / Bridgeman Images

ID: PIX4572490

The smallest stars - Artist's view - The smallest stars. Artwork - Comparison to the scale of the smallest stars with Jupiter and the Sun. From left to right: Jupiter, a brown dwarf (same size as Jupiter but 50 times more massive), dwarf L (younger brown dwarf), red dwarf, Sun. From left to right: Jupiter (a failed star), a brown dwarf (same size as Jupiter but 50 times more massive), a “” L”” dwarf (brown dwarf younger), a red dwarf and the sun for comparison

Artist's view of a star - A sun - like star. Artwork - Artist's view of a star like the Sun. A sun - like star. Artwor
Artist's view of a star - A sun - like star. Artwork - Artist's view of a star like the Sun. A sun - like star. Artwor

PIX4572524: Artist's view of a star - A sun - like star. Artwork - Artist's view of a star like the Sun. A sun - like star. Artwor / Bridgeman Images

ID: PIX4572524

Artist's view of a star - A sun - like star. Artwork - Artist's view of a star like the Sun. A sun - like star. Artwor

Formation of a brown dwarf star - Artist's view - Formation of a brown dwarf star. Artwork - Brown dwarf star shines within its accretion disk. Streams of ionized dust and gas are drawn to the forming star by its magnetic field
Formation of a brown dwarf star - Artist's view - Formation of a brown dwarf star. Artwork - Brown dwarf star shines within its accretion disk. Streams of ionized dust and gas are drawn to the forming star by its magnetic field

PIX4572525: Formation of a brown dwarf star - Artist's view - Formation of a brown dwarf star. Artwork - Brown dwarf star shines within its accretion disk. Streams of ionized dust and gas are drawn to the forming star by its magnetic field, Dixon, Don (b.1951) / Bridgeman Images

ID: PIX4572525

Formation of a brown dwarf star - Artist's view - Formation of a brown dwarf star. Artwork - Brown dwarf star shines within its accretion disk. Streams of ionized dust and gas are drawn to the forming star by its magnetic field

Dixon, Don (b.1951)

Brown dwarf with asteroid ring - Artist's view of a brown dwarf star surrounded by an asteroid belt. In the foreground, a primitive exoplanet illuminated by the star. This brown dwarf is host to a disk composed primarily of asteroids and boulders. The light from this dwarf is barely enough to illuminate the surface of this primitive planet. At a distance of about 1.5 million miles, the orbit of this planet is aligned to the plane of the rings with the result that they appear as a fuzzy line occulting the glowing face of this brown dwarf
Brown dwarf with asteroid ring - Artist's view of a brown dwarf star surrounded by an asteroid belt. In the foreground, a primitive exoplanet illuminated by the star. This brown dwarf is host to a disk composed primarily of asteroids and boulders. The light from this dwarf is barely enough to illuminate the surface of this primitive planet. At a distance of about 1.5 million miles, the orbit of this planet is aligned to the plane of the rings with the result that they appear as a fuzzy line occulting the glowing face of this brown dwarf

PIX4572527: Brown dwarf with asteroid ring - Artist's view of a brown dwarf star surrounded by an asteroid belt. In the foreground, a primitive exoplanet illuminated by the star. This brown dwarf is host to a disk composed primarily of asteroids and boulders. The light from this dwarf is barely enough to illuminate the surface of this primitive planet. At a distance of about 1.5 million miles, the orbit of this planet is aligned to the plane of the rings with the result that they appear as a fuzzy line occulting the glowing face of this brown dwarf / Bridgeman Images

ID: PIX4572527

Brown dwarf with asteroid ring - Artist's view of a brown dwarf star surrounded by an asteroid belt. In the foreground, a primitive exoplanet illuminated by the star. This brown dwarf is host to a disk composed primarily of asteroids and boulders. The light from this dwarf is barely enough to illuminate the surface of this primitive planet. At a distance of about 1.5 million miles, the orbit of this planet is aligned to the plane of the rings with the result that they appear as a fuzzy line occulting the glowing face of this brown dwarf

Brown dwarf with a large debris ring - Artist's view of a brown dwarf star surrounded by a disc of dust and rocks. In the foreground, a primitive exoplanet illuminated by the star. This imaginary high - mass brown dwarf has a larger disk than the previous renderings. The perspective is from the equator of an airless planet, orbiting the brown dwarf at a distance of about 4 million miles. This planet's orbit is very nearly aligned to the plane of the rings, hence the debris appears as a sword - like straight line
Brown dwarf with a large debris ring - Artist's view of a brown dwarf star surrounded by a disc of dust and rocks. In the foreground, a primitive exoplanet illuminated by the star. This imaginary high - mass brown dwarf has a larger disk than the previous renderings. The perspective is from the equator of an airless planet, orbiting the brown dwarf at a distance of about 4 million miles. This planet's orbit is very nearly aligned to the plane of the rings, hence the debris appears as a sword - like straight line

PIX4572539: Brown dwarf with a large debris ring - Artist's view of a brown dwarf star surrounded by a disc of dust and rocks. In the foreground, a primitive exoplanet illuminated by the star. This imaginary high - mass brown dwarf has a larger disk than the previous renderings. The perspective is from the equator of an airless planet, orbiting the brown dwarf at a distance of about 4 million miles. This planet's orbit is very nearly aligned to the plane of the rings, hence the debris appears as a sword - like straight line / Bridgeman Images

ID: PIX4572539

Brown dwarf with a large debris ring - Artist's view of a brown dwarf star surrounded by a disc of dust and rocks. In the foreground, a primitive exoplanet illuminated by the star. This imaginary high - mass brown dwarf has a larger disk than the previous renderings. The perspective is from the equator of an airless planet, orbiting the brown dwarf at a distance of about 4 million miles. This planet's orbit is very nearly aligned to the plane of the rings, hence the debris appears as a sword - like straight line

Paul Francois Jean Nicolas, Viscount de Barras (1755-1829), leader of the Directory. In the uniform of a member of the Executive Board. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.
Paul Francois Jean Nicolas, Viscount de Barras (1755-1829), leader of the Directory. In the uniform of a member of the Executive Board. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.

FLO4572564: Paul Francois Jean Nicolas, Viscount de Barras (1755-1829), leader of the Directory. In the uniform of a member of the Executive Board. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852. / Bridgeman Images

ID: FLO4572564

Paul Francois Jean Nicolas, Viscount de Barras (1755-1829), leader of the Directory. In the uniform of a member of the Executive Board. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.

Artist's view of a nova recurrente - Recurrent nova. Artwork - Artist's view of a nova, a white dwarf star that attracts the material of a companion star at the end of life, a red giant, and compresses these gases and then releases a nuclear fusion reaction releasing a huge amount of energy in the form of a brief, extremely bright light. A nova recurrente is a star with at least two nova-type explosions
Artist's view of a nova recurrente - Recurrent nova. Artwork - Artist's view of a nova, a white dwarf star that attracts the material of a companion star at the end of life, a red giant, and compresses these gases and then releases a nuclear fusion reaction releasing a huge amount of energy in the form of a brief, extremely bright light. A nova recurrente is a star with at least two nova-type explosions

PIX4572573: Artist's view of a nova recurrente - Recurrent nova. Artwork - Artist's view of a nova, a white dwarf star that attracts the material of a companion star at the end of life, a red giant, and compresses these gases and then releases a nuclear fusion reaction releasing a huge amount of energy in the form of a brief, extremely bright light. A nova recurrente is a star with at least two nova-type explosions / Bridgeman Images

ID: PIX4572573

Artist's view of a nova recurrente - Recurrent nova. Artwork - Artist's view of a nova, a white dwarf star that attracts the material of a companion star at the end of life, a red giant, and compresses these gases and then releases a nuclear fusion reaction releasing a huge amount of energy in the form of a brief, extremely bright light. A nova recurrente is a star with at least two nova-type explosions

Nova de l'Eagle - Nova Aquilae. Artwork - Artist's view of a nova, a white dwarf star that attracts the material of a companion star at the end of life, a red giant, and compresses these gases and then unleash a nuclear fusion reaction releasing a huge amount of energy in the form of a brief, extremely bright light. Here the artist showed the binary system just before the explosion of the nova. The artist's illustration depicts a classical nova binary system just before an explosion on the surface of the white dwarf. Classical novas occur in a system where a white dwarf closely orbits a normal, companion star. In this illustration, gas is flowing from the large red, companion star into a disk and then onto the white dwarf that is hidden inside the white area. As the gas flows ever closer to the white dwarf, it gets increasingly hotter, as indicated by the change in colors from yellow to white. When the explosion occurs, it engulfs the disk of gas and the red companion star
Nova de l'Eagle - Nova Aquilae. Artwork - Artist's view of a nova, a white dwarf star that attracts the material of a companion star at the end of life, a red giant, and compresses these gases and then unleash a nuclear fusion reaction releasing a huge amount of energy in the form of a brief, extremely bright light. Here the artist showed the binary system just before the explosion of the nova. The artist's illustration depicts a classical nova binary system just before an explosion on the surface of the white dwarf. Classical novas occur in a system where a white dwarf closely orbits a normal, companion star. In this illustration, gas is flowing from the large red, companion star into a disk and then onto the white dwarf that is hidden inside the white area. As the gas flows ever closer to the white dwarf, it gets increasingly hotter, as indicated by the change in colors from yellow to white. When the explosion occurs, it engulfs the disk of gas and the red companion star

PIX4572591: Nova de l'Eagle - Nova Aquilae. Artwork - Artist's view of a nova, a white dwarf star that attracts the material of a companion star at the end of life, a red giant, and compresses these gases and then unleash a nuclear fusion reaction releasing a huge amount of energy in the form of a brief, extremely bright light. Here the artist showed the binary system just before the explosion of the nova. The artist's illustration depicts a classical nova binary system just before an explosion on the surface of the white dwarf. Classical novas occur in a system where a white dwarf closely orbits a normal, companion star. In this illustration, gas is flowing from the large red, companion star into a disk and then onto the white dwarf that is hidden inside the white area. As the gas flows ever closer to the white dwarf, it gets increasingly hotter, as indicated by the change in colors from yellow to white. When the explosion occurs, it engulfs the disk of gas and the red companion star / Bridgeman Images

ID: PIX4572591

Nova de l'Eagle - Nova Aquilae. Artwork - Artist's view of a nova, a white dwarf star that attracts the material of a companion star at the end of life, a red giant, and compresses these gases and then unleash a nuclear fusion reaction releasing a huge amount of energy in the form of a brief, extremely bright light. Here the artist showed the binary system just before the explosion of the nova. The artist's illustration depicts a classical nova binary system just before an explosion on the surface of the white dwarf. Classical novas occur in a system where a white dwarf closely orbits a normal, companion star. In this illustration, gas is flowing from the large red, companion star into a disk and then onto the white dwarf that is hidden inside the white area. As the gas flows ever closer to the white dwarf, it gets increasingly hotter, as indicated by the change in colors from yellow to white. When the explosion occurs, it engulfs the disk of gas and the red companion star

Costumes of common English people, Directory era. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.
Costumes of common English people, Directory era. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.

FLO4572649: Costumes of common English people, Directory era. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852. / Bridgeman Images

ID: FLO4572649

Costumes of common English people, Directory era. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.

Artist's view of Algol, a binary star has eclipse - Binary system Algol - Artist vie
Artist's view of Algol, a binary star has eclipse - Binary system Algol - Artist vie

PIX4572650: Artist's view of Algol, a binary star has eclipse - Binary system Algol - Artist vie, Dixon, Don (b.1951) / Bridgeman Images

ID: PIX4572650

Artist's view of Algol, a binary star has eclipse - Binary system Algol - Artist vie

Dixon, Don (b.1951)

Stephanie Felicite du Crest de St. Aubin, Countess de Genlis, French writer, harpist and educator 1746-1830. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.
Stephanie Felicite du Crest de St. Aubin, Countess de Genlis, French writer, harpist and educator 1746-1830. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.

FLO4572669: Stephanie Felicite du Crest de St. Aubin, Countess de Genlis, French writer, harpist and educator 1746-1830. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852. / Bridgeman Images

ID: FLO4572669

Stephanie Felicite du Crest de St. Aubin, Countess de Genlis, French writer, harpist and educator 1746-1830. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.

Napoleon Bonaparte, General en Chef, in uniform of General of the Army of Italy, Napoleonic Wars. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.
Napoleon Bonaparte, General en Chef, in uniform of General of the Army of Italy, Napoleonic Wars. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.

FLO4572684: Napoleon Bonaparte, General en Chef, in uniform of General of the Army of Italy, Napoleonic Wars. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852. / Bridgeman Images

ID: FLO4572684

Napoleon Bonaparte, General en Chef, in uniform of General of the Army of Italy, Napoleonic Wars. Handcoloured lithograph from Le Bibliophile Jacob aka Paul Lacroix's Costumes Historique de la France (Historical Costumes of France), Administration de Librairie, Paris, 1852.

Artist's view of an eruptive star - Flare star. Artwork - An eruptive star is a variable star that can manifest a dramatic and imforeseeable increase in luminosite from a few minutes to a few hours. From X-rays to radios, the spectrum increases in intensity. Eruptive stars are red dwarves, although recent research indicates that brown dwarves may also be capable of eruptions. A flare star is a variable star which can undergo unpredictable dramatic increases in brightness for a few minutes or a few hours. The brightness increase is across the spectrum, from X - rays to radio waves. Flare stars are dim red dwarfs, although recent research indicates that brown dwarfs might also be capable of flaring
Artist's view of an eruptive star - Flare star. Artwork - An eruptive star is a variable star that can manifest a dramatic and imforeseeable increase in luminosite from a few minutes to a few hours. From X-rays to radios, the spectrum increases in intensity. Eruptive stars are red dwarves, although recent research indicates that brown dwarves may also be capable of eruptions. A flare star is a variable star which can undergo unpredictable dramatic increases in brightness for a few minutes or a few hours. The brightness increase is across the spectrum, from X - rays to radio waves. Flare stars are dim red dwarfs, although recent research indicates that brown dwarfs might also be capable of flaring

PIX4572699: Artist's view of an eruptive star - Flare star. Artwork - An eruptive star is a variable star that can manifest a dramatic and imforeseeable increase in luminosite from a few minutes to a few hours. From X-rays to radios, the spectrum increases in intensity. Eruptive stars are red dwarves, although recent research indicates that brown dwarves may also be capable of eruptions. A flare star is a variable star which can undergo unpredictable dramatic increases in brightness for a few minutes or a few hours. The brightness increase is across the spectrum, from X - rays to radio waves. Flare stars are dim red dwarfs, although recent research indicates that brown dwarfs might also be capable of flaring, Dixon, Don (b.1951) / Bridgeman Images

ID: PIX4572699

Artist's view of an eruptive star - Flare star. Artwork - An eruptive star is a variable star that can manifest a dramatic and imforeseeable increase in luminosite from a few minutes to a few hours. From X-rays to radios, the spectrum increases in intensity. Eruptive stars are red dwarves, although recent research indicates that brown dwarves may also be capable of eruptions. A flare star is a variable star which can undergo unpredictable dramatic increases in brightness for a few minutes or a few hours. The brightness increase is across the spectrum, from X - rays to radio waves. Flare stars are dim red dwarfs, although recent research indicates that brown dwarfs might also be capable of flaring

Dixon, Don (b.1951)

Artist's view of a fugitive star - A runaway star in the Large Magellanic cloud - The star HE0457 - 5439 is a massive star in the Grand Cloud of Magellan; it is a star escaping from this galaxy at a speed of 2.6 Million km/h Background image obtained at the observatory of La Silla in Chile; the star fleeing has been added on the image. The star HE0457 - 5439 is a massive star wich lies closer to one of the Milky Way satellite galaxies, the Large Magellanic Cloud, located 160,000 light - years away from us. This is a runaway star, moving at more than 2.6 million kilometers per hour. Astronomers find it likely for the star to have reached its present position had it been ejected from the centre of the LMC. The background image has been obtained at La Silla observatory, the star moving has been added
Artist's view of a fugitive star - A runaway star in the Large Magellanic cloud - The star HE0457 - 5439 is a massive star in the Grand Cloud of Magellan; it is a star escaping from this galaxy at a speed of 2.6 Million km/h Background image obtained at the observatory of La Silla in Chile; the star fleeing has been added on the image. The star HE0457 - 5439 is a massive star wich lies closer to one of the Milky Way satellite galaxies, the Large Magellanic Cloud, located 160,000 light - years away from us. This is a runaway star, moving at more than 2.6 million kilometers per hour. Astronomers find it likely for the star to have reached its present position had it been ejected from the centre of the LMC. The background image has been obtained at La Silla observatory, the star moving has been added

PIX4572713: Artist's view of a fugitive star - A runaway star in the Large Magellanic cloud - The star HE0457 - 5439 is a massive star in the Grand Cloud of Magellan; it is a star escaping from this galaxy at a speed of 2.6 Million km/h Background image obtained at the observatory of La Silla in Chile; the star fleeing has been added on the image. The star HE0457 - 5439 is a massive star wich lies closer to one of the Milky Way satellite galaxies, the Large Magellanic Cloud, located 160,000 light - years away from us. This is a runaway star, moving at more than 2.6 million kilometers per hour. Astronomers find it likely for the star to have reached its present position had it been ejected from the centre of the LMC. The background image has been obtained at La Silla observatory, the star moving has been added / Bridgeman Images

ID: PIX4572713

Artist's view of a fugitive star - A runaway star in the Large Magellanic cloud - The star HE0457 - 5439 is a massive star in the Grand Cloud of Magellan; it is a star escaping from this galaxy at a speed of 2.6 Million km/h Background image obtained at the observatory of La Silla in Chile; the star fleeing has been added on the image. The star HE0457 - 5439 is a massive star wich lies closer to one of the Milky Way satellite galaxies, the Large Magellanic Cloud, located 160,000 light - years away from us. This is a runaway star, moving at more than 2.6 million kilometers per hour. Astronomers find it likely for the star to have reached its present position had it been ejected from the centre of the LMC. The background image has been obtained at La Silla observatory, the star moving has been added

Two Girls consulting a Gipsy Fortune-teller
Two Girls consulting a Gipsy Fortune-teller

USB1162976: Two Girls consulting a Gipsy Fortune-teller, English School, (19th century) / Bridgeman Images

ID: USB1162976

Two Girls consulting a Gipsy Fortune-teller

English School, (19th century)

An Unknown Lady (oil on canvas)
An Unknown Lady (oil on canvas)

USB1162980: An Unknown Lady (oil on canvas), Riley, John (1646-91) (attr. to) / Bridgeman Images

ID: USB1162980

An Unknown Lady (oil on canvas)

Riley, John (1646-91) (attr. to)

The Rt Hon. William Windham III MP (1750-1810)
The Rt Hon. William Windham III MP (1750-1810)

USB1162982: The Rt Hon. William Windham III MP (1750-1810), English School / Bridgeman Images

ID: USB1162982

The Rt Hon. William Windham III MP (1750-1810)

English School

A Bearded Man in Oriental Costume (in the manner of Rembrandt)
A Bearded Man in Oriental Costume (in the manner of Rembrandt)

USB1162997: A Bearded Man in Oriental Costume (in the manner of Rembrandt), English School, (18th century) / Bridgeman Images

ID: USB1162997

A Bearded Man in Oriental Costume (in the manner of Rembrandt)

English School, (18th century)

An Unknown Gentleman
An Unknown Gentleman

USB1162998: An Unknown Gentleman, English School, (19th century) / Bridgeman Images

ID: USB1162998

An Unknown Gentleman

English School, (19th century)

The Meeting of Abraham and Melchizedek
The Meeting of Abraham and Melchizedek

USB1163000: The Meeting of Abraham and Melchizedek, Heins, John Theodore, Sr. (1697-1756) / Bridgeman Images

ID: USB1163000

The Meeting of Abraham and Melchizedek

Heins, John Theodore, Sr. (1697-1756)

Cremer Cremer (1768-1808)
Cremer Cremer (1768-1808)

USB1163001: Cremer Cremer (1768-1808), English School, (19th century) / Bridgeman Images

ID: USB1163001

Cremer Cremer (1768-1808)

English School, (19th century)

A View of Norwich Castle
A View of Norwich Castle

USB1163007: A View of Norwich Castle, Catton, Charles, II (1756-1819) / Bridgeman Images

ID: USB1163007

A View of Norwich Castle

Catton, Charles, II (1756-1819)

River Scene at Night (oil on copper)
River Scene at Night (oil on copper)

USB1163010: River Scene at Night (oil on copper), English School, (18th century) / Bridgeman Images

ID: USB1163010

River Scene at Night (oil on copper)

English School, (18th century)

A Norfolk Beach Scene (oil on canvas)
A Norfolk Beach Scene (oil on canvas)

USB1163015: A Norfolk Beach Scene (oil on canvas), Stannard, Joseph (1797-1830) / Bridgeman Images

ID: USB1163015

A Norfolk Beach Scene (oil on canvas)

Stannard, Joseph (1797-1830)

Four British Warships and a Fishing-smack in a Strong Wind
Four British Warships and a Fishing-smack in a Strong Wind

USB1163018: Four British Warships and a Fishing-smack in a Strong Wind, Monamy, Peter (1681-1749) / Bridgeman Images

ID: USB1163018

Four British Warships and a Fishing-smack in a Strong Wind

Monamy, Peter (1681-1749)

A Whaler and other Ships at Anchor before a Port
A Whaler and other Ships at Anchor before a Port

USB1163019: A Whaler and other Ships at Anchor before a Port, Storck, Abraham (1644-1708) / Bridgeman Images

ID: USB1163019

A Whaler and other Ships at Anchor before a Port

Storck, Abraham (1644-1708)

John Ketton (1808-1872)
John Ketton (1808-1872)

USB1163027: John Ketton (1808-1872), English School, (19th century) / Bridgeman Images

ID: USB1163027

John Ketton (1808-1872)

English School, (19th century)

Sailing Boats on a Calm Sea (oil on canvas)
Sailing Boats on a Calm Sea (oil on canvas)

USB1163029: Sailing Boats on a Calm Sea (oil on canvas), Jodrell (19th century) / Bridgeman Images

ID: USB1163029

Sailing Boats on a Calm Sea (oil on canvas)

Jodrell (19th century)

Mary Queen of Scots returning to Scotland from France passing the Cliffs of Dover
Mary Queen of Scots returning to Scotland from France passing the Cliffs of Dover

USB1163032: Mary Queen of Scots returning to Scotland from France passing the Cliffs of Dover, English School, (19th century) / Bridgeman Images

ID: USB1163032

Mary Queen of Scots returning to Scotland from France passing the Cliffs of Dover

English School, (19th century)

South Front of Felbrigg Hall, Norfolk
South Front of Felbrigg Hall, Norfolk

USB1163034: South Front of Felbrigg Hall, Norfolk, English School, (20th century) / Bridgeman Images

ID: USB1163034

South Front of Felbrigg Hall, Norfolk

English School, (20th century)

Thomas Cremer
Thomas Cremer

USB1163038: Thomas Cremer, English School / Bridgeman Images

ID: USB1163038

Thomas Cremer

English School

An Unknown Lady
An Unknown Lady

USB1163042: An Unknown Lady, English School / Bridgeman Images

ID: USB1163042

An Unknown Lady

English School

Icon of the Madonna and Child with Four Saints
Icon of the Madonna and Child with Four Saints

USB1163055: Icon of the Madonna and Child with Four Saints, Russian School / Bridgeman Images

ID: USB1163055

Icon of the Madonna and Child with Four Saints

Russian School

The Doge's Palace and Piazzetta San Marco, Venice (imitator of Canaletto)
The Doge's Palace and Piazzetta San Marco, Venice (imitator of Canaletto)

USB1163056: The Doge's Palace and Piazzetta San Marco, Venice (imitator of Canaletto), English School, (19th century) / Bridgeman Images

ID: USB1163056

The Doge's Palace and Piazzetta San Marco, Venice (imitator of Canaletto)

English School, (19th century)


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