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The X-ray emission and the magnetic fields of late-type stars
Shi, JR; Zhao, G; Zhao, Y
2002
Source PublicationASTROPHYSICS AND SPACE SCIENCE
Volume282Issue:3Pages:477-488
AbstractWe present the results of X-ray luminosities of some active late-type stars, based on data primarily from the ROSAT position sensitive proportional counter (PSPC). According to the observations, we divide the stars into four groups: single, wide binary, binary and RS CVn. We investigated the correlation between the X-ray emission and the hardness ratio, coronal temperature, magnetic field strength, magnetic flux density. Our results suggest that the magnetic field plays a very important role in stellar X-ray emission.
Indexed BySCI
Language英语
WOS IDWOS:000178955600002
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8507
Collection光学天文研究部
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.Chinese Acad Sci Peking Univ Joint Beijing Astrop, Beijing 100871, Peoples R China
Recommended Citation
GB/T 7714
Shi, JR,Zhao, G,Zhao, Y. The X-ray emission and the magnetic fields of late-type stars[J]. ASTROPHYSICS AND SPACE SCIENCE,2002,282(3):477-488.
APA Shi, JR,Zhao, G,&Zhao, Y.(2002).The X-ray emission and the magnetic fields of late-type stars.ASTROPHYSICS AND SPACE SCIENCE,282(3),477-488.
MLA Shi, JR,et al."The X-ray emission and the magnetic fields of late-type stars".ASTROPHYSICS AND SPACE SCIENCE 282.3(2002):477-488.
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