File:M51 CHANDRA2.jpg
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Summary
[edit]The Whirlpool Galaxy (also known as Messier 51, M51, or NGC 5194) is a classic spiral galaxy located in the Canes Venatici constellation. It was discovered by Charles Messier on October 13, 1773.
- X-rays from a rare type of supernova in the Whirlpool Galaxy were recently observed, thanks to the fine resolution of NASA's Chandra X-ray Observatory. The team of researchers also detected a large number of point-like X-ray sources due to black holes and neutron stars in binary star systems.
- Chandra's image highlights the energetic central regions of the two interacting galaxies, NGC 5194 (center) and its smaller companion (upper left) NGC 5195, that are collectively called the Whirlpool Galaxy.
http://www.msfc.nasa.gov/news/news/photos/2002/photos02-163.html (Credit: NASA/CXC/UMD/A. Wilson et al.)
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current | 14:32, 19 November 2005 | 1,926 × 1,473 (113 KB) | Makary (talk | contribs) | M51 im promieniach rentgena http://www.msfc.nasa.gov/news/news/photos/2002/photos02-163.html (Credit: NASA/CXC/UMD/A. Wilson et al.) |
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