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Immagini di ' Si Chiama Cosi'' trovate, 26

Socalled

Socalled

WWL3893622

Do You Know: Why is grapefruit so called? (colour litho)

Do You Know: Why is grapefruit so called? (colour litho)

English School, (20th century)

LLM8668107

The girl with such coy style is named Darling Moncada, one of over 5,000 Nicaraguan refugees in Los Guasimo camp in Honduras; child playing with an umbrella, 1987-03-06 (photo)

The girl with such coy style is named Darling Moncada, one of over 5,000 Nicaraguan refugees in Los Guasimo camp in Honduras; child playing with an umbrella, 1987-03-06 (photo)

Hayward, Anthony

REU11969117

The Calling of St Matthew, 1530s (oil on panel)

The Calling of St Matthew, 1530s (oil on panel)

Mertens, Jan the Younger (c.1470-c.1527)

ROC452140

Cast photograph of "Mrs Dot", July 1918 (b/w photo)

Cast photograph of "Mrs Dot", July 1918 (b/w photo)

BRV8599273

BEWICK / ORANG-UTAN

BEWICK / ORANG-UTAN

EPL6932080

SYMPATHETIC MAGIC

SYMPATHETIC MAGIC

Picart, Bernard (1673-1733)

EPL6815175

SHREW (BEWICK)

EPL6894060

Rainbow - Rainbow - Rainbow - Arc - en - ciel observed in Brittany on 2 May 2005. 23 minutes before the sun sets, a contrasting rainbow appears in the east. It is very high (the lower the Sun, the higher the bow). Note at the level of the “feet” of the rainbow the difference in luminosite between the interior of the rainbow (under the main arch) and the band between the main arch and the secondary arch (lower and higher). This dark band is called Alexander's Band. It should also be noted that blue is almost absent from the rainbow, because the Sun is setting, therefore orange, betrays a blue light faults that can be seen at the level of the rainbow. May 2, 2005. 23 minutes before the sunset, a contrasted rainbow appear toward the East. It's a tall rainbow, because the Sun is low. Notice the difference of luminosity at the “” feet”” of the rainbow between the inside of the rainbow (under the main arc) and the band located between the main and secondary arcs (fainter and higher). This darker band is called the Alexander's dark band. Notice too that the blue tints are missing in the rainbow, because the sun is setting, so is orange, which means that its blue tints are absent — Rainbow - Rainbow - Rainbow - Arc - en - ciel observed in Brittany on 2 May 2005. 23 minutes before the sun sets, a contrasting rainbow appears in the east. It is very high (the lower the Sun, the higher the bow). Note at the level of the “feet” of the rainbow the difference in luminosite between the interior of the rainbow (under the main arch) and the band between the main arch and the secondary arch (lower and higher). This dark band is called Alexander's Band. It should also be noted that blue is almost absent from the rainbow, because the Sun is setting, therefore orange, betrays a blue light faults that can be seen at the level of the rainbow. May 2, 2005. 23 minutes before the sunset, a contrasted rainbow appear toward the East. It's a tall rainbow, because the Sun is low. Notice the difference of luminosity at the “” feet”” of the rainbow between the inside of the rainbow (under the main arc) and the band located between the main and secondary arcs (fainter and higher). This da

Rainbow - Rainbow - Rainbow - Arc - en - ciel observed in Brittany on 2 May 2005. 23 minutes before the sun sets, a contrasting rainbow appears in the east. It is very high (the lower the Sun, the higher the bow). Note at the level of the “feet” of the rainbow the difference in luminosite between the interior of the rainbow (under the main arch) and the band between the main arch and the secondary arch (lower and higher). This dark band is called Alexander's Band. It should also be noted that blue is almost absent from the rainbow, because the Sun is setting, therefore orange, betrays a blue light faults that can be seen at the level of the rainbow. May 2, 2005. 23 minutes before the sunset, a contrasted rainbow appear toward the East. It's a tall rainbow, because the Sun is low. Notice the difference of luminosity at the “” feet”” of the rainbow between the inside of the rainbow (under the main arc) and the band located between the main and secondary arcs (fainter and higher). This da

Laurent Laveder

PIX4671117

Ferruccio Parri and Antonio De Caro smoke a cigarette while walking, Italy

Ferruccio Parri and Antonio De Caro smoke a cigarette while walking, Italy

MEP2502414

Books and Scholars’ Accoutrements (ink & colour on silk)

Books and Scholars’ Accoutrements (ink & colour on silk)

Yi Taek-gyun (1808- after 1883)

XCL5846775

Chinese Fiddles

Chinese Fiddles

EPL7019066

Switzerland Agriculture Irrigation, 1972 (b/w photo)

Switzerland Agriculture Irrigation, 1972 (b/w photo)

Fritz Grunder

KES6207895

Open cluster NGC 4755 - Jewel Box - The Jewel Box star cluster - The NGC 4755 cluster is located in the constellation of the Southern Cross at a distance of 6400 years - light from Earth. The bright orange star on the top right is Kappa Crucis, a supergiant red star. This cluster contains about fifty stars formed about 16 million years ago. This close-up of the center of the cluster was obtained with the Hubble Space Telescope. This image is a “” close - up 'view from the NASA/ESA Hubble Space Telescope of NGC 4755, or the Jewel Box cluster. Several very bright, pale blue supergiant stars, a solitary ruby - red supergiant and a variety of other brilliantly coloured stars are visible in the image, as well as many much fainter ones, often with intriguing colours. The huge variety in brightness exists because the brighter stars are 15 to 20 times the mass of the Sun, while the dimmest stars are less than half the mass of the Sun. This is the first image of an open galactic cluster with imaging extending from the far ultraviolet to the near - infrared. NGC 4755 (Caldwell 94) is called the Jewel Box, based on John Herschel's comment in the 1830's that it looked like a superb piece of jewelry. There are about 50 stars in this cluster which formed some 14 million years ago. Most of the cluster members are blue giants which in a few million years will exhaust their hydrogen fuel and become red giants on their way to a cataclysmic end as supernovae. One red giant can already be seen at the center of the cluster (top right) — Open cluster NGC 4755 - Jewel Box - The Jewel Box star cluster - The NGC 4755 cluster is located in the constellation of the Southern Cross at a distance of 6400 years - light from Earth. The bright orange star on the top right is Kappa Crucis, a supergiant red star. This cluster contains about fifty stars formed about 16 million years ago. This close-up of the center of the cluster was obtained with the Hubble Space Telescope. This image is a “” close - up 'view from the NASA/ESA Hubble Space Telescope of NGC 4755, or the Jewel Box cluster. Several very bright, pale blue supergiant stars, a solitary ruby - red supergiant and a variety of other brilliantly coloured stars are visible in the image, as well as many much fainter ones, often with intriguing colours. The huge variety in brightness exists because the brighter stars are 15 to 20 times the mass of the Sun, while the dimmest stars are less than half the mass of the Sun. This is the first image of an open galactic cluster with im

Open cluster NGC 4755 - Jewel Box - The Jewel Box star cluster - The NGC 4755 cluster is located in the constellation of the Southern Cross at a distance of 6400 years - light from Earth. The bright orange star on the top right is Kappa Crucis, a supergiant red star. This cluster contains about fifty stars formed about 16 million years ago. This close-up of the center of the cluster was obtained with the Hubble Space Telescope. This image is a “” close - up 'view from the NASA/ESA Hubble Space Telescope of NGC 4755, or the Jewel Box cluster. Several very bright, pale blue supergiant stars, a solitary ruby - red supergiant and a variety of other brilliantly coloured stars are visible in the image, as well as many much fainter ones, often with intriguing colours. The huge variety in brightness exists because the brighter stars are 15 to 20 times the mass of the Sun, while the dimmest stars are less than half the mass of the Sun. This is the first image of an open galactic cluster with im

PIX4568246

Bugler of the Seventeenth, Undress (lithograph)

Bugler of the Seventeenth, Undress (lithograph)

Hull, Edward (19th century) (after)

NAM5929045

Looking at the new Photographic Technology

Looking at the new Photographic Technology

UIG2900920

Coral-Reefs', 1849

Coral-Reefs', 1849

UIS5090601

China: 'Mencius - The Three Moves', anon., 20th century

China: 'Mencius - The Three Moves', anon., 20th century

Unknown Artist, (20th century)

PFH3085471

Hochmeisterstein in memory of Ulrich von Jungingen

Hochmeisterstein in memory of Ulrich von Jungingen

Scherl

SZT5175532

Martin Gutzeit, 1990 (photo)

Martin Gutzeit, 1990 (photo)

SZT11775335

Nepal: An image of the Hindu goddess Kali, Bhaktapur, Kathmandu Valley (1996) (photo)

Nepal: An image of the Hindu goddess Kali, Bhaktapur, Kathmandu Valley (1996) (photo)

Rainer Krack

PFH2641697

The lost sheep (colour litho)

The lost sheep (colour litho)

Beard, Frank (1842-1905)

LLM11702122

Lieutenant James Noyce (d. 1813), c.1800 (watercolour, ivory, gilt, pearl, glass, hair, opal)

Lieutenant James Noyce (d. 1813), c.1800 (watercolour, ivory, gilt, pearl, glass, hair, opal)

Unknown Artist, (19th century)

MMM7340104

Rotterdam, Holland (b/w photo)

Rotterdam, Holland (b/w photo)

American Photographer, (19th century)

LLM11732666

Palace of Fontainebleau, France (b/w photo)

Palace of Fontainebleau, France (b/w photo)

American Photographer, (19th century)

LLM11701134

Codex Selden / Codex Añute, c. 1560 (manuscript)

Codex Selden / Codex Añute, c. 1560 (manuscript)

BDL9031249

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