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摘要

描述
English: M82, at a distance of 11 million light years from Earth, is the nearest starburst galaxy. Massive stars are forming and expiring in M82 at a rate ten times higher than in our galaxy. The bright spots in the center are supernova remnants and X-ray binaries. These are some of the brightest such objects known. The luminosity of the X-ray binaries suggests that most contain a black hole. The diffuse X-ray light in the image extends over several thousand light years, and is caused by multimillion degree gas flowing out of M82. A close encounter with a large galaxy, M81, in the last 100 million years is thought to be the cause of the starburst activity.
日期 2000年1月14日 (上傳日期)
來源 M82: Chandra Images Seething Cauldron of Starburst Galaxy - http://www.seds.org/messier/more/m082_cxo.html
作者 NASA/CXC/SAO/PSU/CMU
其他版本
Also Known As
InfoField
Cigar Galaxy
Category
InfoField
Normal Galaxies & Starburst Galaxies, Black Holes
Color Code
InfoField
Hot pink dots - the rest is intensity
Constellation
InfoField
Ursa Major
Coordinates (J2000)
InfoField
RA 09h 55m 50.70s
Distance Estimate
InfoField
12 million light years
Observation Date(s)
InfoField
September 20, 1999
Observation ID(s)
InfoField
361, 1302
Observation Time
InfoField
13 hours
Scale
InfoField
Image is 5 arcmin across.
Instruments
InfoField
ACIS
This media is a product of the
Chandra X-ray Observatory
Credit and attribution belongs to the Chandra X-ray Center, NASA/SAO/Penn State University/MIT

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Public domain 本作品由NASA創作,屬於公有領域。根據NASA的版權政策:“NASA的創作除非另有聲明否則不受版權保護。”(參見:Template:PD-USGov/zhNASA版權政策JPL圖像使用政策
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Transferred from en.wikipedia to Commons using FtCG.

The original description page was here. All following user names refer to en.wikipedia.
Date/Time Dimensions User Comment
00:09, 17 August 2005 510 × 509 (84,246 bytes) w:en:Uber nemo (對話 | 貢獻) (http://www.seds.org/messier/more/m082_cxo.html {{PD-USGov-NASA}})

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