Soft X-ray emission of nearby galaxy M81
文献类型:期刊论文
作者 | Su, Y![]() |
刊名 | SCIENCE IN CHINA SERIES A-MATHEMATICS
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出版日期 | 1997 |
卷号 | 40期号:1页码:93-104 |
关键词 | spiral galaxy nearby galaxy soft X-ray emission |
英文摘要 | The pointed observations of NGC3077 are analyzed by position sensitive proportional counter (PSPC) board the ROSAT satellite on 1991-04-18, 1991, finding out that the X-ray emission range of M81 galaxy has, in the softer and more sensitive ROSAT PSPC band (0.2-2.4 keV), extended by 40% larger than ever observed by image proportional counter (IPC) on board the Einstein satellite, which shows that M81 galaxy has a larger X-ray corona. And by the aid of the timing analysis, it is concluded that M81 nucleus has no variabilities on time scale of a few minutes; hence the possibility of M81 nucleus having the marginal variability over time scale of about 2 min that Fabbiano (1988) found from the Einstein IPC observation is ruled out. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:A1997WJ37000011 |
源URL | [http://ir.bao.ac.cn/handle/114a11/8325] ![]() |
专题 | 国家天文台_月球与深空探测研究部 |
作者单位 | 1.UNIV ARIZONA, DEPT PHYS, TUCSON, AZ 85716 USA 2.CHINESE ACAD SCI, BEIJING ASTRON OBSERV, BEIJING 100080, PEOPLES R CHINA |
推荐引用方式 GB/T 7714 | Su, Y,Bi, HG,Li, QB. Soft X-ray emission of nearby galaxy M81[J]. SCIENCE IN CHINA SERIES A-MATHEMATICS,1997,40(1):93-104. |
APA | Su, Y,Bi, HG,&Li, QB.(1997).Soft X-ray emission of nearby galaxy M81.SCIENCE IN CHINA SERIES A-MATHEMATICS,40(1),93-104. |
MLA | Su, Y,et al."Soft X-ray emission of nearby galaxy M81".SCIENCE IN CHINA SERIES A-MATHEMATICS 40.1(1997):93-104. |
入库方式: OAI收割
来源:国家天文台
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