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3101. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B2CA6C300-1FC8-4B17-BCA3-95E922A1989C%7D
. The low-mass binary pair is tethered by a weak gravitational link that results in an orbital dance so slow that it takes about 500,000 years to complete a single revolution. Gemini Observatory/Cerro Tololo/2MASS/DSS
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B2CA6C300-1FC8-4B17-BCA3-95E922A1989C%7D -- 3.1 Кб -- 10.04.2016
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3102. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B29EC70D5-2855-4F84-9523-2D017A40F52F%7D
. This Hubble Space Telescope composite image shows a ghostly "ring" of dark matter in the galaxy cluster ZwCl0024+1652. NASA, ESA, M.J. Jee and H. Ford (Johns Hopkins University)
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B29EC70D5-2855-4F84-9523-2D017A40F52F%7D -- 3.1 Кб -- 10.04.2016
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3103. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B18944F14-1D83-403C-929C-B7B9510A168D%7D
. This high-resolution image captures the details of an elongated tendril of gas pouring out of the Crab Nebula supernova remnant. Although the image was not taken as part of any ongoing research project, astronomers have found it useful in their study of expanding nebulae. Subaru Telescope
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B18944F14-1D83-403C-929C-B7B9510A168D%7D -- 3.3 Кб -- 10.04.2016
[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B8D26E673-6FC1-4EA9-8C44-C4F95174F403%7D -- 3.3 Кб -- 10.04.2016
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[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B8D26E673-6FC1-4EA9-8C44-C4F95174F403%7D -- 3.3 Кб -- 10.04.2016
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3104. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B161FD368-A7EF-4765-AACD-9F0010FBF408%7D
. A 10-billion-degree cloud of nuclear ash erupts from a white dwarf in this computer simulation. Alan Calder, Univ. of Chicago
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B161FD368-A7EF-4765-AACD-9F0010FBF408%7D -- 2.9 Кб -- 10.04.2016
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3105. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0C07A0E5-7A82-4944-B343-E1214BC0DED0%7D
. Many gathered at Kitt Peak Visitor's Center to observe the Sun. Robert D. Miller
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0C07A0E5-7A82-4944-B343-E1214BC0DED0%7D -- 2.9 Кб -- 10.04.2016
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3106. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF6CF0261-7C34-49B5-8CCE-FB30CCAC3C9C%7D
. New Hubble observations suggest that I Zwicky 18 is 59 million light-years from Earth, almost 10 million light-years more distant than previously believed. NASA, ESA and A. Aloisi (ESA/STScI)
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF6CF0261-7C34-49B5-8CCE-FB30CCAC3C9C%7D -- 3.1 Кб -- 10.04.2016
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3107. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF3470500-A3D2-45E4-9963-EE48D6847155%7D
. Galaxy NGC 4395 contains an intermediate-mass black hole about 400,000 times more massive than the Sun. Such a black hole may have evolved into the supermassive black holes seen throughout the universe today. David W. Hogg/Michael R. Blanton/Sloan Digital Sky Survey Collaboration
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF3470500-A3D2-45E4-9963-EE48D6847155%7D -- 3.3 Кб -- 10.04.2016
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3108. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BC332368F-FD5D-4AAF-8905-205618B205EB%7D
. This VLBI image of the inner region of galaxy NGC 4395 shows extended radio emission that indicates suspected outflow powered by an intermediate-mass black hole. Wrobel & Ho/NRAO/AUI/NSF
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BC332368F-FD5D-4AAF-8905-205618B205EB%7D -- 3.1 Кб -- 10.04.2016
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3109. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB618B898-D3EC-472F-840A-62C452D7028B%7D
. VLBI image of the inner region of galaxy NGC 4395, showing extended radio emission that indicates suspected outflow powered by an intermediate-mass black hole. Wrobel & Ho, NRAO/AUI/NSF
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB618B898-D3EC-472F-840A-62C452D7028B%7D -- 3.1 Кб -- 10.04.2016
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3110. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BAD050464-A4D3-4212-93A0-E66A97190E7A%7D
. The bright globular cluster M15 is easy to see in binoculars. It houses what seems to be the first interstellar gas ever found in a globular cluster. NASA and The Hubble Heritage Team (STScI/AURA)
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BAD050464-A4D3-4212-93A0-E66A97190E7A%7D -- 3.1 Кб -- 10.04.2016
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3111. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BA3B3BA95-8BAB-49B2-B6F4-AAF52C71F00E%7D
. This artist's impression shows a galaxy located between an observer on Earth and a background quasar that acts as a beacon. The light that travels from the quasar is intercepted by the foreground galaxy on its sightline, carrying out the galaxy's signature all the way to the observer. The sketch shows a side-on view of the system. The inset shows a face-on view of it, the same view captured (albeit with less detail) by the images taken with the SINFONI instrument on ESO's Very Large Telescope. ESO
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BA3B3BA95-8BAB-49B2-B6F4-AAF52C71F00E%7D -- 3.8 Кб -- 10.04.2016
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3112. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B82D7A9F3-B5E3-426A-A939-B2C80B135EF8%7D
. This new Subaru image used in the study was released in March 2007. By measuring the proper motion of the supernova debris across the plane of the sky over 17 years, this group of astronomers was able to confirm the 1054 explosion date. Subaru Telescope
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B82D7A9F3-B5E3-426A-A939-B2C80B135EF8%7D -- 3.2 Кб -- 10.04.2016
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3113. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B828538E5-4F43-4EEE-896A-412C103C10B7%7D
. This view shows a color composite image of the gravitational lens system, made from Hubble (blue and green) and Keck (red) data. The blue ring is the tiny background galaxy, stretched by the gravitational pull of the foreground lens galaxy at the center of the image. Marshall & Treu (UCSB)
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B828538E5-4F43-4EEE-896A-412C103C10B7%7D -- 3.3 Кб -- 10.04.2016
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3114. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B7B65EB6A-2626-47B6-A8BA-A1BCCFE08CCB%7D
. Cosmic rays have been traced to the cores of nearby galaxies. The image above shows a spiral galaxy. NASA / JPL-Caltech / S. Willner (Harvard-Smithsonian CfA)
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B7B65EB6A-2626-47B6-A8BA-A1BCCFE08CCB%7D -- 3.0 Кб -- 10.04.2016
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3115. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B2D6F44C8-BCF5-4E45-B9EC-A508028FB9CE%7D
. This image is an artist's rendition of HD 141569A's disk. Subaru Telescope, NAOJ
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B2D6F44C8-BCF5-4E45-B9EC-A508028FB9CE%7D -- 2.8 Кб -- 10.04.2016
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3116. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1841E2D8-21B3-4F91-AC19-BF22C7A79301%7D
. Eta Carinae is located about 7,500 light-years from Earth. In the 1840s, Eta Carinae survived a massive eruption, briefly becoming the second brightest star in the sky. The latest composite image from NASA's Chandra X-ray Observatory and the Hubble Space Telescope shows remnants of that titanic event, hinting that the star may be nearing its final, massive explosion. X-ray: NASA/CXC/GSFC/M. Corcoran et al; Optical: NASA/STScl
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1841E2D8-21B3-4F91-AC19-BF22C7A79301%7D -- 3.6 Кб -- 10.04.2016
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3117. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF092343C-70F3-422E-BBF8-14FE798024F2%7D
. A white dwarf, shown in the bottom right of this artist's impression, accretes material from a red giant, which is losing gas in the form of stellar wind. Only part of the gas is accreted by the white dwarf through a disk that surrounds the compact star. The remaining gas escapes the system and eventually dissipates into the interstellar medium. ESO
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF092343C-70F3-422E-BBF8-14FE798024F2%7D -- 3.5 Кб -- 10.04.2016
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3118. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BEF720739-4A19-4A2A-9AB7-94F3C2A7BAB4%7D
. In this false-color image, blue represents aurora emissions from hydrogen gas excited by electron bombardment, while red-orange represents reflected sunlight. NASA / JPL / University of Colorado
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BEF720739-4A19-4A2A-9AB7-94F3C2A7BAB4%7D -- 3.1 Кб -- 10.04.2016
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3119. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD64B7380-1723-44C8-80CD-93563B5B688D%7D
. CERN will beam trillions of neutrinos under Earth's surface to a detector in Italy's Gran Sasso National Laboratory. Cern diagram
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD64B7380-1723-44C8-80CD-93563B5B688D%7D -- 3.0 Кб -- 10.04.2016
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3120. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BC6EE7665-9593-4DC1-80BC-53282D332828%7D
. This image shows a 2-D spectrum obtained in 92 hours of exposure time, showing the line emitter candidates. The quasar absorption lines are visible close to the center of the image. ESO
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BC6EE7665-9593-4DC1-80BC-53282D332828%7D -- 3.1 Кб -- 10.04.2016
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