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3181. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3085040D-5CB1-412C-A0E8-EE1D093B86DF%7D
. This image shows water vapor-clouds (in shades of blue) in S Persei, observed using MERLIN. The doppler shifts of the maser spectral lines mean astronomers can measure the speed and direction of the wind blown away from the star. RAS
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3085040D-5CB1-412C-A0E8-EE1D093B86DF%7D -- 3.2 Кб -- 10.04.2016
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3182. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B002AF218-9639-4B82-BC4D-15675FA3509A%7D
. This is a triple gravitational lens, an example of the rich diversity of the 67 strong gravitational lenses found in the COSMOS survey. NASA/ESA/C. Faure/J.P. Kneib
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B002AF218-9639-4B82-BC4D-15675FA3509A%7D -- 3.0 Кб -- 10.04.2016
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3183. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF17903F8-1635-4F9D-BFED-A8BD0595830E%7D
. The cluster Collinder 261, which scientists used to observe dozens of red giants. Digitized Sky Survey
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF17903F8-1635-4F9D-BFED-A8BD0595830E%7D -- 2.9 Кб -- 10.04.2016
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3184. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE93C62C8-5AC5-40C6-BA1F-8E9B00F35FB1%7D
. Very-high-energy gamma rays are arranged in a thick band across the Milky WayтАЩs center. The gamma rays are likely a result of accelerated cosmic rays. HESS project
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE93C62C8-5AC5-40C6-BA1F-8E9B00F35FB1%7D -- 3.0 Кб -- 10.04.2016
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3185. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD7846158-46E8-4010-9B6C-6E6731C6D2A9%7D
. This SOHO image shows a coronal mass ejection blasting off the Sun. NASA
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD7846158-46E8-4010-9B6C-6E6731C6D2A9%7D -- 2.8 Кб -- 10.04.2016
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3186. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B91CC0CC7-B6B0-4A85-966E-AF857E586485%7D
. After performing a mathematical computation known as a Fourier analysis, scientists can extract a quasi-periodic signal (light echoes) from what appears to be random noise. Keigo Fukumura
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B91CC0CC7-B6B0-4A85-966E-AF857E586485%7D -- 3.1 Кб -- 10.04.2016
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3187. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B89D10491-ECDE-4A58-8818-11F6AC4F0594%7D
. About 75% of a flareтАЩs X-rays (black line) head toward Earth without completing an orbit. But the remainder orbit the black hole one or more times (red, blue, green, pink, and orange lines) before heading our way. Keigo Fukumura
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B89D10491-ECDE-4A58-8818-11F6AC4F0594%7D -- 3.2 Кб -- 10.04.2016
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3188. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B7080ACD7-62FD-4440-8ADD-78FF4DC14851%7D
. This ground-based image shows globular cluster NGC 6397. D. Verschatse (Antilhue Observatory, Chile)
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B7080ACD7-62FD-4440-8ADD-78FF4DC14851%7D -- 2.9 Кб -- 10.04.2016
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3189. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5C6B9CF0-37BF-4B48-A8F4-CD02EFD4DB2A%7D
. The barred spiral galaxy NGC 1672 shows clusters of hot, young, blue stars along its spiral arms, and clouds of hydrogen gas glowing in red. Delicate curtains of dust partially obscure and redden the light of the stars behind them. NASA/ESA
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5C6B9CF0-37BF-4B48-A8F4-CD02EFD4DB2A%7D -- 3.2 Кб -- 10.04.2016
[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B9AD7B4B3-95DE-44E1-931C-EC737C3C3B4A%7D -- 3.2 Кб -- 10.04.2016
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[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B9AD7B4B3-95DE-44E1-931C-EC737C3C3B4A%7D -- 3.2 Кб -- 10.04.2016
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3190. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B588BBDAF-40A9-4713-996D-F1C415A96AC2%7D
. This Hubble Space Telescope image shows globular cluster NGC 6397. NASA/ESA/H. Richer (University of British Columbia)
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B588BBDAF-40A9-4713-996D-F1C415A96AC2%7D -- 2.9 Кб -- 10.04.2016
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3191. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B48AEFDA3-3F17-46BC-B24D-DF225CEE4BEB%7D
. The Chandra X-ray Observatory imaged Sagittarius A East, the supernova remnant at the galaxy's center. The remnant is the yellowish area in the center, and surrounds white dots — the Milky Way's supermassive black hole Sagittarius A*. NASA / Penn State / G.Garmire et al.
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B48AEFDA3-3F17-46BC-B24D-DF225CEE4BEB%7D -- 3.3 Кб -- 10.04.2016
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3192. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B479D6C12-02F2-4ADE-AB36-4A335D352CB1%7D
. An X-ray observatory will receive large numbers of signals from multiple flares, and the signals will appear at first glance to be totally random. Keigo Fukumura
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B479D6C12-02F2-4ADE-AB36-4A335D352CB1%7D -- 3.0 Кб -- 10.04.2016
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3193. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B2BA36FA3-4854-4A08-B39B-DDA118C3FE1B%7D
. An observer will see multiple X-ray signals from the same flare, with the timing evenly spaced for the X-rays that completed one or more orbits around the black hole. These repeating signals are light echoes. Keigo Fukumura
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B2BA36FA3-4854-4A08-B39B-DDA118C3FE1B%7D -- 3.2 Кб -- 10.04.2016
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3194. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B239FAE2F-5F71-4150-86BE-0C9EBB4C6A20%7D
. This 2005 image of NGC 1300, another barred spiral galaxy, shows starlight, glowing gas, and silhouetted dark clouds of interstellar dust. Barred spirals differ from normal spiral galaxies in that the arms of the galaxy do not spiral all the way into the center, but are connected to the two ends of a straight bar of stars containing the nucleus at its center. NASA/Hubble/STScI/AURA
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B239FAE2F-5F71-4150-86BE-0C9EBB4C6A20%7D -- 3.5 Кб -- 10.04.2016
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3195. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B199D4D25-7511-4AA6-ADB7-FCC7C8A5FC2D%7D
. This artist's impression shows gas within a "sphere of influence" falling straight inwards towards a black hole before joining a rapidly spinning disk of matter near the center. NASA/CXC/M.Weiss
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B199D4D25-7511-4AA6-ADB7-FCC7C8A5FC2D%7D -- 3.1 Кб -- 10.04.2016
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3196. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1295436A-2FAD-4900-BCF8-E17A3FC1F972%7D
. This artist rendition shows an accretion disk swirling around a black hole. The two hot spots could give off powerful X-ray flares. NASA/Dana Berry, SkyWorks Digital
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1295436A-2FAD-4900-BCF8-E17A3FC1F972%7D -- 3.0 Кб -- 10.04.2016
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3197. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0919B4DC-640B-4C8B-9D8E-26BE765110B4%7D
. This illustration shows a close-up view of a supermassive black hole in a galaxy's center. NASA/CXC/M.Weiss
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0919B4DC-640B-4C8B-9D8E-26BE765110B4%7D -- 2.9 Кб -- 10.04.2016
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3198. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BED901423-44DB-46CE-93BA-50ACBBE1A1FA%7D
. This Mars Odyssey image, taken in 2002, shows the upper portion of the Ganges Chasma landslide. NASA/JPL
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BED901423-44DB-46CE-93BA-50ACBBE1A1FA%7D -- 2.9 Кб -- 10.04.2016
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3199. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE1618CD2-2FEC-439C-8DB9-85C8E39ED46E%7D
. In this top-down illustration of a black hole and its surrounding disk, gas spiraling toward the black hole piles up just outside it, creating a traffic jam. The traffic jam is closer in for smaller black holes, so X-rays are emitted on a shorter timescale. NASA
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE1618CD2-2FEC-439C-8DB9-85C8E39ED46E%7D -- 3.3 Кб -- 10.04.2016
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3200. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBE9D4FA2-E5FF-4E7A-A836-3D94DAC5BACD%7D
. This illustration shows the distribution of dark matter, massive halos, and luminous quasars in a simulation of the early universe, shown 1.6 billion years after the Big Bang. Gray filaments show the distribution of dark matter. Small white circles mark concentrated "halos" of dark matter. Larger blue circles mark the most massive halos, which host the most luminous quasars. Paul Bode/Yue Shen, Princeton University
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBE9D4FA2-E5FF-4E7A-A836-3D94DAC5BACD%7D -- 3.6 Кб -- 10.04.2016
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