NAOC Open IR  > 光学天文研究部
Magnetic fields in active late-type stars
Shi, JR; Zhao, G; Zhao, YH
AbstractThe very high resolution and high signal-to-noise ratio spectra of ten x-ray selected stars are obtained by the NAOC Coude spectrograph. Magnetic field measurements of these stars have been performed using the profile-addition technique. The magnetic field strength and filling factor are obtained, and we End that there exist strong magnetic fields on very active stars.
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WOS IDWOS:000178755700049
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Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
AffiliationChinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Recommended Citation
GB/T 7714
Shi, JR,Zhao, G,Zhao, YH. Magnetic fields in active late-type stars[J]. CHINESE PHYSICS LETTERS,2002,19(10):1560-1561.
APA Shi, JR,Zhao, G,&Zhao, YH.(2002).Magnetic fields in active late-type stars.CHINESE PHYSICS LETTERS,19(10),1560-1561.
MLA Shi, JR,et al."Magnetic fields in active late-type stars".CHINESE PHYSICS LETTERS 19.10(2002):1560-1561.
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