中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
On the soft X-ray emission of M82

文献类型:期刊论文

作者Liu, J.1; Wang, Q. D.2; Mao, S.1,3
刊名ASTRONOMISCHE NACHRICHTEN
出版日期2012-04-01
卷号333期号:4页码:365-368
关键词atomic processes galaxies: individual (M82) galaxies: starburst X-rays: galaxies
英文摘要We present a spatial analysis of the soft X-ray and H alpha emissions from the outflow of the starburst galaxy M82. We find that the two emissions are tightly correlated on various scales. The O VII triplet of M82, as resolved by X-ray grating observations of XMM-Newton, is dominated by the forbidden line, inconsistent with the thermal prediction. The O VII triplet also shows some spatial variations. We discuss three possible explanations for the observed O VII triplet, including the charge exchange at interfaces between the hot outflow and neutral cool gas, a collisional non-equilibrium-ionization recombining plasma, and resonance scattering. (c) 2012 WILEY-VCH Verlag GmbH&Co. KGaA, Weinheim
收录类别SCI
语种英语
WOS记录号WOS:000305329700017
源URL[http://ir.bao.ac.cn/handle/114a11/6289]  
专题国家天文台_应用天文研究部
作者单位1.Natl Astron Observ, Beijing 100012, Peoples R China
2.Univ Massachusetts, Dept Astron, Amherst, MA 01002 USA
3.Univ Manchester, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, England
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GB/T 7714
Liu, J.,Wang, Q. D.,Mao, S.. On the soft X-ray emission of M82[J]. ASTRONOMISCHE NACHRICHTEN,2012,333(4):365-368.
APA Liu, J.,Wang, Q. D.,&Mao, S..(2012).On the soft X-ray emission of M82.ASTRONOMISCHE NACHRICHTEN,333(4),365-368.
MLA Liu, J.,et al."On the soft X-ray emission of M82".ASTRONOMISCHE NACHRICHTEN 333.4(2012):365-368.

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来源:国家天文台

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