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AstroSam

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http://chandra.harvard.edu/graphics/top/wsn/bg.jpg



A Precocious Black Hole

Credit: Illustration: M. Helfenbein, Yale University / OPAC
http://chandra.harvard.edu/photo/2015/cid947/cid947_525.jpg
Researchers have discovered a black hole that grew much more quickly than its host galaxy. The discovery calls into question previous assumptions on the development of galaxies. The black hole was originally discovered using NASA's Hubble Space Telescope, and was then detected in the Sloan Digital Sky Survey and by ESA's XMM-Newton and NASA's Chandra X-ray Observatory.
 

ratfeast

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Researchers have discovered a black hole that grew much more quickly than its host galaxy. The discovery calls into question previous assumptions on the development of galaxies. The black hole was originally discovered using NASA's Hubble Space Telescope, and was then detected in the Sloan Digital Sky Survey and by ESA's XMM-Newton and NASA's Chandra X-ray Observatory.
I don't understand how it could do that; is the galaxy being eaten by the black hole?

I didn't realize the horsehead Nebula was that large! Nice picture.
 
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AstroSam

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Reflection Nebula in Orion: NGC 1999
Widefield shot:

http://annesastronomynews.com/wp-content/uploads/2012/02/NGC-1999-widefield-by-Robert-Gendler.jpg
Zoomed shot:

http://apod.nasa.gov/apod/image/0003/ngc1999_hst_big.jpg
The nebula, cataloged as NGC 1999, is a reflection nebula, which shines by reflecting light from a nearby star.(...) NGC 1999's stellar illumination is provided by the embedded variable star V380 Orionis, seen here just left of center. Extending right of center, the ominous dark nebula is actually a condensation of cold molecular gas and dust so thick and dense that it blocks light.(...) Reflection nebula NGC 1999 lies about 1500 light-years away in the constellation Orion, just south of Orion's well known emission nebula, M42.
http://apod.nasa.gov/apod/ap000302.html
 

AstroSam

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The Boomerang Nebula is a young planetary nebula and the coldest object found in the Universe so far. The NASA/ESA Hubble Space Telescope image is yet another example of how Hubble's sharp eye reveals surprising details in celestial objects.(...)With a temperature of -272C, it is only 1 degree warmer than absolute zero (the lowest limit for all temperatures). Even the -270C background glow from the Big Bang is warmer than this nebula. It is the only object found so far that has a temperature lower than the background radiation.
View: https://www.spacetelescope.org/images/heic0301a/


https://cdn.spacetelescope.org/archives/images/thumb700x/heic0301a.jpg

Magellanic Cloud: The tip of the "wing" of the Small Magellanic Cloud galaxy is dazzling in this new view from NASA's Great Observatories. The Small Magellanic Cloud, or SMC, is a small galaxy about 200,000 light-years way that orbits our own Milky Way spiral galaxy.

http://www.nasa.gov/images/content/738996main_pia16884-43_946-710.jpg
(...)The SMC is one of the Milky Way's closest galactic neighbors. Even though it is a small, or so-called dwarf galaxy, the SMC is so bright that it is visible to the unaided eye from the Southern Hemisphere and near the equator. Many navigators, including Ferdinand Magellan who lends his name to the SMC, used it to help find their way across the oceans.(...)
View: http://www.nasa.gov/mission_pages/spitzer/multimedia/pia16884.html
 

AstroSam

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Supernova NGC 6888:

http://3.bp.blogspot.com/--1_qUbzWwYc/T5EfZc8sMVI/AAAAAAAAGUI/2u4qIIN4YTs/s1600/CrescentHa-OIIIDLopez_n.jpg
NGC 6888, also known as the Crescent Nebula, is a cosmic bubble about 25 light-years across, blown by winds from its central, bright, massive star.(...)NGC 6888's central star is classified as a Wolf-Rayet star (WR 136). The star is shedding its outer envelope in a strong stellar wind, ejecting the equivalent of the Sun's mass every 10,000 years. The nebula's complex structures are likely the result of this strong wind interacting with material ejected in an earlier phase. Burning fuel at a prodigious rate and near the end of its stellar life this star should ultimately go out with a bang in a spectacular supernova explosion.(...)
View: http://apod.nasa.gov/apod/ap120816.html
 

AstroSam

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AstroSam

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Our solar eclipse corona in detailed views:


http://images.astronet.ru/pubd/2010/03/16/0001239639/corona_druckmuller.jpg


http://www.ifa.hawaii.edu/info/press-releases/2015solar_eclipse/druckmuller_SolarCorona_TSE2015_Svalbard.jpg


Explanation: Only in the fleeting darkness of a total solar eclipse is the light of the solar corona easily visible. Normally overwhelmed by the bright solar disk, the expansive corona, the sun's outer atmosphere, is an alluring sight. But the subtle details and extreme ranges in the corona's brightness, although discernible to the eye, are notoriously difficult to photograph.
More: http://www.astronet.ru/db/xware/msg/apod/2010-03-16
 
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