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Images of 'La Banda' found, 23,554

 
Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 distant about 16 million years - light in the constellation Lynx. Image obtained by the Hubble Space Telescope (HST). NGC 2683 is a spiral galaxy seen almost edge - on, giving it the shape of a classic science fiction spaceship. The delicate dusty lanes of the spiral arms are silhouetted against the golden haze of the galaxy's core. In addition, brilliant clusters of young blue stars shine scattered throughout the disc, mapping the galaxy's star - forming regions. Perhaps surprisingly, side - on views of galaxies like this one do not prevent astronomers from deducing their structures. Studies of the properties of the light coming from NGC 2683 suggest that this is a barred spiral galaxy, even though the angle we see it at does not let us see this directly. NGC 2683, discovered on 5 February 1788 by the famous astronomer William Herschel, lies in the Northern constellation of Lynx. A constellation n

PIX4610165

Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 distant about 16 million years - light in the constellation Lynx. Image obtained by the Hubble Space Telescope (HST). NGC 2683 is a spiral galaxy seen almost edge - on, giving it the shape of a classic science fiction spaceship. The delicate dusty lanes of the spiral arms are silhouetted against the golden haze of the galaxy's core. In addition, brilliant clusters of young blue stars shine scattered throughout the disc, mapping the galaxy's star - forming regions. Perhaps surprisingly, side - on views of galaxies like this one do not prevent astronomers from deducing their structures. Studies of the properties of the light coming from NGC 2683 suggest that this is a barred spiral galaxy, even though the angle we see it at does not let us see this directly. NGC 2683, discovered on 5 February 1788 by the famous astronomer William Herschel, lies in the Northern constellation of Lynx. A constellation n

PIX4610165

 
Centaurus A elliptical galaxy (NGC 5128) in Centaurus - The radio galaxy Centaurus A (NGC 5128): The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. - NGC 5128 is the nearest large elliptical galaxies to our sun at about 13 million light years. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky. In 1949, NGC 5128 was found to be a loud source of radio energy, in fact the loudest radio source in its region of the sky (second overall to Cygnus A), earning it the designation Centarus A. As a radio galaxy it releases 1000 times the radio energy of the Milky Way in the form of large bi

PIX4612309

Centaurus A elliptical galaxy (NGC 5128) in Centaurus - The radio galaxy Centaurus A (NGC 5128): The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. - NGC 5128 is the nearest large elliptical galaxies to our sun at about 13 million light years. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky. In 1949, NGC 5128 was found to be a loud source of radio energy, in fact the loudest radio source in its region of the sky (second overall to Cygnus A), earning it the designation Centarus A. As a radio galaxy it releases 1000 times the radio energy of the Milky Way in the form of large bi

PIX4612309

 
Centaurus A Elliptical Galaxy (NGC 5128) in the Centaur - Galaxy Centaurus A - The NGC 5128 galaxy is about 11 million years away - light from Earth. This image from the Hubble Space Telescope (HST) shows the star flames that occur in the dark band of the galaxy. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. Centaurus A, also known as NGC 5128, is well known for its dramatic dusty lanes of dark material. Hubble's observations, using its most advanced instrument, the Wide Field Camera 3, are the most detailed ever made of this galaxy. They have been combined here in a multi - wavelength image that reveals never - before - seen detail in the dusty portion of the galaxy. As well as features in the visible spectrum, this composite shows ultraviolet light from young stars, and near - infrared light, which lets us glimpse some of the detail otherwise obscured by the dust. The dark dust lane that cr

PIX4612191

Centaurus A Elliptical Galaxy (NGC 5128) in the Centaur - Galaxy Centaurus A - The NGC 5128 galaxy is about 11 million years away - light from Earth. This image from the Hubble Space Telescope (HST) shows the star flames that occur in the dark band of the galaxy. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. Centaurus A, also known as NGC 5128, is well known for its dramatic dusty lanes of dark material. Hubble's observations, using its most advanced instrument, the Wide Field Camera 3, are the most detailed ever made of this galaxy. They have been combined here in a multi - wavelength image that reveals never - before - seen detail in the dusty portion of the galaxy. As well as features in the visible spectrum, this composite shows ultraviolet light from young stars, and near - infrared light, which lets us glimpse some of the detail otherwise obscured by the dust. The dark dust lane that cr

PIX4612191

 
Heart of the Nebula of the Lagoon (M8) in Sagittarius seen by HST - This NASA Hubble Space Telescope (HST) image reveals a pair of one - half light - year long interstellar “” twisters”” - - eerie funnels and twisted - rope structures (upper left) - - in the heart of the Lagoon Nebula (Messier 8) which lies 5,000 years - - away in the direction of the constellation Sagittarius. The central hot O type star, Herschel 36 (upper left in photo), is the primary source of the ionizing radiation for the brightest region in the nebula, called the Hourglass. Other hot stars, also present in the nebula, are ionizing the extended optical nebulosity. The ionizing radiation induces photo - evaporation of the surfaces of the clouds (seen as a blue “” mist”” at the right of the image), and drives away violent stellar winds tearing into the cool clouds.Analogous to the spectacular phenomena of Earth tornadoes, the large difference in temperature between the hot surface and cold interior of the clouds,

PIX4619680

Heart of the Nebula of the Lagoon (M8) in Sagittarius seen by HST - This NASA Hubble Space Telescope (HST) image reveals a pair of one - half light - year long interstellar “” twisters”” - - eerie funnels and twisted - rope structures (upper left) - - in the heart of the Lagoon Nebula (Messier 8) which lies 5,000 years - - away in the direction of the constellation Sagittarius. The central hot O type star, Herschel 36 (upper left in photo), is the primary source of the ionizing radiation for the brightest region in the nebula, called the Hourglass. Other hot stars, also present in the nebula, are ionizing the extended optical nebulosity. The ionizing radiation induces photo - evaporation of the surfaces of the clouds (seen as a blue “” mist”” at the right of the image), and drives away violent stellar winds tearing into the cool clouds.Analogous to the spectacular phenomena of Earth tornadoes, the large difference in temperature between the hot surface and cold interior of the clouds,

PIX4619680

 
Planetary nebula NGC 6302 in Scorpio - Planetary nebula NGC 6302 in Scorpius - NGC 6302 is a planetary nebula located about 4000 years from Earth. In the center of the nebula, an extremely hot dying star. Image obtained by the Hubble Space Telescope with the new WFC 3 (Wide Field Camera 3) camera, July 27, 2009. A dying star that was once about five times the mass of the Sun is at the center of this nebula. It has ejected its envelope of gases and is now unleashing a stream of ultraviolet radiation that is making the cast - off material glow. This object is an example of a planetary nebula, so - named because many of them have a round appearance resembling that of a planet when viewed through a small telescope. The Wide Field Camera 3 (WFC3), a new camera aboard Nasa's Hubble Space Telescope, snapped this image of the planetary nebula, catalogued as NGC 6302, but more popularly called the Bug Nebula or the Butterfly Nebula. WFC3 was installed by NASA astronauts in May 2009, during the

PIX4623200

Planetary nebula NGC 6302 in Scorpio - Planetary nebula NGC 6302 in Scorpius - NGC 6302 is a planetary nebula located about 4000 years from Earth. In the center of the nebula, an extremely hot dying star. Image obtained by the Hubble Space Telescope with the new WFC 3 (Wide Field Camera 3) camera, July 27, 2009. A dying star that was once about five times the mass of the Sun is at the center of this nebula. It has ejected its envelope of gases and is now unleashing a stream of ultraviolet radiation that is making the cast - off material glow. This object is an example of a planetary nebula, so - named because many of them have a round appearance resembling that of a planet when viewed through a small telescope. The Wide Field Camera 3 (WFC3), a new camera aboard Nasa's Hubble Space Telescope, snapped this image of the planetary nebula, catalogued as NGC 6302, but more popularly called the Bug Nebula or the Butterfly Nebula. WFC3 was installed by NASA astronauts in May 2009, during the

PIX4623200

 
The galactic center seen by Spitzer Space Telescope - The galactic center region seen by Spitzer satellite. The area photographed extends over 890 light-years and over 640 light-years high. In visible light, this area is hidden by a large amount of interstellar dust. This picture in false colors shows the old and cold stars in blue, and the red regions the hot and massive stars. Dark and bright filamentous clouds are star-forming regions. The brightest area in the center of the image is the center of our galaxy which houses a supermassive black hole. This infrared image from Nasa's Spitzer Space Telescope shows hundreds of thousands of stars crowded into the swirling core of our spiral Milky Way galaxy. In visible-light pictures, this region cannot be seen at all because dust lying between Earth and the galactic center blocks our view. In this false-color picture, old and cool stars are blue, while dust features lit up by blazing hot, massive stars are shown in a reddish hue. Both brig

PIX4637936

The galactic center seen by Spitzer Space Telescope - The galactic center region seen by Spitzer satellite. The area photographed extends over 890 light-years and over 640 light-years high. In visible light, this area is hidden by a large amount of interstellar dust. This picture in false colors shows the old and cold stars in blue, and the red regions the hot and massive stars. Dark and bright filamentous clouds are star-forming regions. The brightest area in the center of the image is the center of our galaxy which houses a supermassive black hole. This infrared image from Nasa's Spitzer Space Telescope shows hundreds of thousands of stars crowded into the swirling core of our spiral Milky Way galaxy. In visible-light pictures, this region cannot be seen at all because dust lying between Earth and the galactic center blocks our view. In this false-color picture, old and cool stars are blue, while dust features lit up by blazing hot, massive stars are shown in a reddish hue. Both brig

PIX4637936

 
Map of the sky seen by Planck - The microwave sky as seen by Planck - 380,000 years after the formation of the universe, when the temperature had become low enough, the light could be released from the extremely dense material that imprisoned it and spread throughout the universe. This moment appears to us today in the form of a radiation called fossil radiation, or cosmological diffuse background. This image is the map of temperature fluctuations of the cosmological diffuse background (in orange) seen by the Planck satellite between August 2009 and June 2010. Overlay, in blue, the Lactee Way and clear, filamentary structures that extend beyond the plane of our Lactee Way. This multi-frequency all-sky image of the microwave sky has been composed using data from Planck covering the electromagnetic spectrum from 30 GHz to 857 GHz. The mottled structure of the CMBR, with its tiny temperature fluctuations reflecting the primordial density variations from which today's cosmic structure orig

PIX4634312

Map of the sky seen by Planck - The microwave sky as seen by Planck - 380,000 years after the formation of the universe, when the temperature had become low enough, the light could be released from the extremely dense material that imprisoned it and spread throughout the universe. This moment appears to us today in the form of a radiation called fossil radiation, or cosmological diffuse background. This image is the map of temperature fluctuations of the cosmological diffuse background (in orange) seen by the Planck satellite between August 2009 and June 2010. Overlay, in blue, the Lactee Way and clear, filamentary structures that extend beyond the plane of our Lactee Way. This multi-frequency all-sky image of the microwave sky has been composed using data from Planck covering the electromagnetic spectrum from 30 GHz to 857 GHz. The mottled structure of the CMBR, with its tiny temperature fluctuations reflecting the primordial density variations from which today's cosmic structure orig

PIX4634312

 
Centaurus A Elliptical Galaxy (NGC 5128) in the Centaur - Galaxy Centaurus A - The NGC 5128 galaxy is about 13 million years away - light from Earth. This image obtained by the Hubble Space Telescope in 1998 shows the star flames that occur in the dark band of the galaxy. In blue, these are the clusters of newly shaped young stars. At the top left, a photo of the galaxy obtained from the ground. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. NGC 5128 is the nearest large elliptical galaxies to our sun. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky. Among many other things NGC 5128 is also the prototypical postmerger elliptical galaxy. Structural peculiarities including the prominent rotating disk of stars and gas and the complex shell structure of its halo point to a large scale merger

PIX4612157

Centaurus A Elliptical Galaxy (NGC 5128) in the Centaur - Galaxy Centaurus A - The NGC 5128 galaxy is about 13 million years away - light from Earth. This image obtained by the Hubble Space Telescope in 1998 shows the star flames that occur in the dark band of the galaxy. In blue, these are the clusters of newly shaped young stars. At the top left, a photo of the galaxy obtained from the ground. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. NGC 5128 is the nearest large elliptical galaxies to our sun. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky. Among many other things NGC 5128 is also the prototypical postmerger elliptical galaxy. Structural peculiarities including the prominent rotating disk of stars and gas and the complex shell structure of its halo point to a large scale merger

PIX4612157

 
Far Galaxies - Chandra Deep Field South - Distant Galaxies - GOODS Chandra Deep Field South - A myriad of distant galaxies, accompanied by a few stars of our Lactee Way, covers almost the entire picture. Some detected galaxies are a billion times weaker than the human eye can perceive without instrument. Many new galaxies are so distant that they appear to us as they were when the Universe was only two billion years old. The image was made by the Very Large Telescope and the 2.2m telescope of La Silla within the framework of the GOODS programme, an extensive programme of study of primordial galaxies conducted by different terrestrial and spatial observatories, in a field of the boreal constellation of the Great Bear and in a field of the southern hemisphere, as here in the constellation of the Furnace. November 2008. Obtained in part with the Very Large Telescope, the image contains more than 27 million pixels and is the result of 55 hours of observations with the VIMOS instrument. Thi

PIX4613813

Far Galaxies - Chandra Deep Field South - Distant Galaxies - GOODS Chandra Deep Field South - A myriad of distant galaxies, accompanied by a few stars of our Lactee Way, covers almost the entire picture. Some detected galaxies are a billion times weaker than the human eye can perceive without instrument. Many new galaxies are so distant that they appear to us as they were when the Universe was only two billion years old. The image was made by the Very Large Telescope and the 2.2m telescope of La Silla within the framework of the GOODS programme, an extensive programme of study of primordial galaxies conducted by different terrestrial and spatial observatories, in a field of the boreal constellation of the Great Bear and in a field of the southern hemisphere, as here in the constellation of the Furnace. November 2008. Obtained in part with the Very Large Telescope, the image contains more than 27 million pixels and is the result of 55 hours of observations with the VIMOS instrument. Thi

PIX4613813

 
Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC 6205), extends for about 150 years - light and is approximately 25,000 years - light from Earth in the constellation of Hercules. Image obtained by the Hubble Space Telescope. M13 is home to over 100,000 stars and located at a distance of 25,000 light - years. These stars are packed so closely together in a ball, approximately 150 light - years across, that they will spend their entire lives whirling around in the cluster. Near the core of this cluster, the density of stars is about a hundred times greater than the density in the neighborhood of our sun. These stars are so crowded that they can, at times, slam into each other and even form a new star, called a “blue straggler.” The brightest reddish stars in the cluster are ancient red giants. These aging stars have expanded to many times their original diameters and cooled. The blue - white stars are the hottest in the cluster. Globular clu

PIX4564696

Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC 6205), extends for about 150 years - light and is approximately 25,000 years - light from Earth in the constellation of Hercules. Image obtained by the Hubble Space Telescope. M13 is home to over 100,000 stars and located at a distance of 25,000 light - years. These stars are packed so closely together in a ball, approximately 150 light - years across, that they will spend their entire lives whirling around in the cluster. Near the core of this cluster, the density of stars is about a hundred times greater than the density in the neighborhood of our sun. These stars are so crowded that they can, at times, slam into each other and even form a new star, called a “blue straggler.” The brightest reddish stars in the cluster are ancient red giants. These aging stars have expanded to many times their original diameters and cooled. The blue - white stars are the hottest in the cluster. Globular clu

PIX4564696

 
Centaurus A elliptical galaxy (NGC 5128) in Centaurus - The radio galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. Image obtained with a 35 cm telescope, 11 hours of cumulative poses. NGC 5128 is the nearest large elliptical galaxies to our sun at about 13 million light years. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky. In 1949, NGC 5128 was found to be a loud source of radio energy, in fact the loudest radio source in its region of the sky (second overall to Cygnus A), earning it the designation Centarus A. As a radio galaxy it releases 1000 t

R. Gendler

PIX4612271

Centaurus A elliptical galaxy (NGC 5128) in Centaurus - The radio galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. Image obtained with a 35 cm telescope, 11 hours of cumulative poses. NGC 5128 is the nearest large elliptical galaxies to our sun at about 13 million light years. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky. In 1949, NGC 5128 was found to be a loud source of radio energy, in fact the loudest radio source in its region of the sky (second overall to Cygnus A), earning it the designation Centarus A. As a radio galaxy it releases 1000 t

R. Gendler

PIX4612271

 
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Tribute to the Victims of the attacks in Paris 2015

IMO2546862

Tribute to the Victims of the attacks in Paris 2015

IMO2546862

 
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Sallet, c.1510 (medium-carbon steel, quenched and tempered)

German School, (16th century)

TWC5862302

Sallet, c.1510 (medium-carbon steel, quenched and tempered)

German School, (16th century)

TWC5862302

 
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Sallet, c.1510 (medium-carbon steel, quenched and tempered)

German School, (16th century)

TWC5862306

Sallet, c.1510 (medium-carbon steel, quenched and tempered)

German School, (16th century)

TWC5862306

 
Fromings Collection: Production of Malawi Darkfired Tobacco Part 4 1956

BAF8619154

Fromings Collection: Production of Malawi Darkfired Tobacco Part 4 1956

BAF8619154

 
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Figure 3: Head-dress of white satin. One purple and two white feathers placed in the bandeau on the left side. The hair, light frizzed, thrown into easy curls, falling over the bandeau. Long ear-rings of pearls. One string of pearls and one chain of gold round the neck. The petticoat of white satin, embroidered in colours. A Circassian robe, of purple and orange-striped satin; the train cut in bias and rounded. The corset of white satin, with long sleeves of the same, tied round the wrist with two purple ribands. The short-sleeves of the robe, and the robe itself trimmed with fur... Figure 4: A Scotch bonnet of garnet-coloured satin, the ends trimmed with a gold fringe, and the bonnet with blue fox fur; a heron feather of gold on the left side. Chemise of clear-worked muslin, trimmed round the neck with a broad lace, and flounced with white fringe; long close sleeves, equally trimmed with lace, and tied with garnet-coloured riband; over them loose sleeves. The sash of a broad garnet-co

BL3294757

Figure 3: Head-dress of white satin. One purple and two white feathers placed in the bandeau on the left side. The hair, light frizzed, thrown into easy curls, falling over the bandeau. Long ear-rings of pearls. One string of pearls and one chain of gold round the neck. The petticoat of white satin, embroidered in colours. A Circassian robe, of purple and orange-striped satin; the train cut in bias and rounded. The corset of white satin, with long sleeves of the same, tied round the wrist with two purple ribands. The short-sleeves of the robe, and the robe itself trimmed with fur... Figure 4: A Scotch bonnet of garnet-coloured satin, the ends trimmed with a gold fringe, and the bonnet with blue fox fur; a heron feather of gold on the left side. Chemise of clear-worked muslin, trimmed round the neck with a broad lace, and flounced with white fringe; long close sleeves, equally trimmed with lace, and tied with garnet-coloured riband; over them loose sleeves. The sash of a broad garnet-co

BL3294757

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