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Bilder zu 'Puntando Verso L'alto' gefunden, 12

An Italian soldier of the Machine Gun Battalion in Spain, shown aiming a machine gun upwards (b/w photo)

An Italian soldier of the Machine Gun Battalion in Spain, shown aiming a machine gun upwards (b/w photo)

FAF493855

Study of two male figures (red chalk on paper) (verso)

Study of two male figures (red chalk on paper) (verso)

Buonarroti, Michelangelo (1475-1564)

BAL191798

Illustration from 'Kaidash's Family", Ivan Nechuy-Levytsky, 1878, 1974 (gouache on paper)

premium — Illustration from 'Kaidash's Family", Ivan Nechuy-Levytsky, 1878, 1974 (gouache on paper)

Illustration from 'Kaidash's Family", Ivan Nechuy-Levytsky, 1878, 1974 (gouache on paper)

Tsarevich, Ivan (1908-92)

AGC6204716

Holbeins Dance of Death: The Beggar (engraving)

Holbeins Dance of Death: The Beggar (engraving)

Holbein the Younger, Hans (1497/8-1543) (after)

LLM5221224

The Conversion of Saul, c.1800 (pen & ink and w/c on wove paper)

The Conversion of Saul, c.1800 (pen & ink and w/c on wove paper)

Blake, William (1757-1827)

HEH5854526

St. Margaret in a Landscape : A Sybil, c.1580-1609 (metal under glass)

St. Margaret in a Landscape : A Sybil, c.1580-1609 (metal under glass)

Carracci, Annibale (1560-1609) (after)

WES7240836

Noli Me Tangere, c.1645-1713 (oil on canvas)

Noli Me Tangere, c.1645-1713 (oil on canvas)

Maratta or Maratti, Carlo (1625-1713) (follower of)

WES7240849

Koo Stark pointing agun in a scene from Agatha Christie's play And Then There Were None, 1988-02-03 (photo)

Koo Stark pointing agun in a scene from Agatha Christie's play And Then There Were None, 1988-02-03 (photo)

Peter Skingley

REU11952702

Balboa discovers the Pacific

Balboa discovers the Pacific

EPL7012400

Arnoldo Foà during a theatre play

Arnoldo Foà during a theatre play

Agenzia Pitre

MEP2364271

Brazilian president elect Fernando Collor de Mello with former SEc. of State Henry Kissinger and Chairman of Americas society David Rockefeller at the Society, NYC, 1990-01-25 (photo)

Brazilian president elect Fernando Collor de Mello with former SEc. of State Henry Kissinger and Chairman of Americas society David Rockefeller at the Society, NYC, 1990-01-25 (photo)

Stubblebine, Ray

REU12002049

Nebuleuse N44 in the Great Magellan Cloud - This photo shows the southern part of the spectacular N44 region in the Large Magellanic Cloud. The green colour indicates areas that are particularly hot. The field measures 27.5 x 26.5 arcmin2., North is up and East is left. The two best known satellite galaxies of the Milky Way, the Magellanic Clouds, are located in the southern sky at a distance of about 170,000 light - years. They host many giant nebular complexes with very hot and luminous stars whose intense ultraviolet radiation causes the surrounding interstellar gas to glow. The intricate and colourful nebulae are produced by ionised gas that shines as electrons and positively charged atomic nuclei recombine, emitting a cascade of photons at well defined wavelengths. Such nebulae are called “” H II regions””, signifying ionised hydrogen, i.e. hydrogen atoms that have lost one electron (protons). Their spectra are characterized by emission lines whose relative intensities carry useful information about the composition of the emitting gas, its temperature, as well as the mechanisms that cause the ionization. Since the wavelengths of these spectral lines correspond to different colours, these alone are already very informative about the physical conditions of the gas. N44 in the Large Magellanic Cloud is a spectacular example of such a giant H II region. Having observed it in 1999 a team of European astronomers again used the Wide - Field - Imager (WFI) at the MPG/ESO 2.2 - m telescope of the La Silla Observatory, pointing this 67 - million pixel digital camera to the same sky region in order to provide another striking - and scientifically extremely rich - image of this complex of nebulae. With a size of roughly 1,000 light - years, the peculiar shape of N44 clearly outlines a ring that includes a bright stellar association of about 40 very luminous and bluish stars. These stars are the origin of powerful “” stellar winds””” that blow away the surrounding gas, pilin — Nebuleuse N44 in the Great Magellan Cloud - This photo shows the southern part of the spectacular N44 region in the Large Magellanic Cloud. The green colour indicates areas that are particularly hot. The field measures 27.5 x 26.5 arcmin2., North is up and East is left. The two best known satellite galaxies of the Milky Way, the Magellanic Clouds, are located in the southern sky at a distance of about 170,000 light - years. They host many giant nebular complexes with very hot and luminous stars whose intense ultraviolet radiation causes the surrounding interstellar gas to glow. The intricate and colourful nebulae are produced by ionised gas that shines as electrons and positively charged atomic nuclei recombine, emitting a cascade of photons at well defined wavelengths. Such nebulae are called “” H II regions””, signifying ionised hydrogen, i.e. hydrogen atoms that have lost one electron (protons). Their spectra are characterized by emission lines whose relative intensities carry usefu

Nebuleuse N44 in the Great Magellan Cloud - This photo shows the southern part of the spectacular N44 region in the Large Magellanic Cloud. The green colour indicates areas that are particularly hot. The field measures 27.5 x 26.5 arcmin2., North is up and East is left. The two best known satellite galaxies of the Milky Way, the Magellanic Clouds, are located in the southern sky at a distance of about 170,000 light - years. They host many giant nebular complexes with very hot and luminous stars whose intense ultraviolet radiation causes the surrounding interstellar gas to glow. The intricate and colourful nebulae are produced by ionised gas that shines as electrons and positively charged atomic nuclei recombine, emitting a cascade of photons at well defined wavelengths. Such nebulae are called “” H II regions””, signifying ionised hydrogen, i.e. hydrogen atoms that have lost one electron (protons). Their spectra are characterized by emission lines whose relative intensities carry usefu

PIX4620812

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