中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Surface Map of the RS CVn-type Star UX Arietis

文献类型:会议论文

作者Gu SH(顾盛宏); Tan HS(谭徽松); Wang XB(王晓彬); Dan HG(单红光); Gu SH(顾盛宏); Dan HG(单红光); Tan HS(谭徽松); Wang XB(王晓彬)
出版日期2004
会议名称the 219th symposium of the International Astronomical Union held during the IAU General Assembly XXV
会议日期2003-07-21
会议地点Sydney, Australia
卷号219
页码873-877
英文摘要New high-resolution spectroscopic observation of RS CVn-type binary UX Ari made in Feb. 2000 is analyzed by means of Doppler imaging technique. The well-known code DoTS is applied to the FeI6430.844 and CaI6439.075 lines and a surface map of the K0IV component of the binary system is derived. The result has demonstrated that the main features of the map are two high-latitude (about 70 degree) spot active regions separated about 120 degree. In addition a middle-latitude weak spot and an equator belt weak spot are also appeared in the map. Such a spot structure pattern is related to the feature of the chromospheric activity of UX Ari in Feb. 2000.
收录类别SCI
产权排序第一完成单位
会议网址http://adsabs.harvard.edu/abs/2004IAUS..219..873G
会议录Proceedings of the 219th symposium of the International Astronomical Union held during the IAU General Assembly XXV - Stars as suns : activity, evolution and planets
学科主题天文学
语种英语
源URL[http://ir.ynao.ac.cn/handle/114a53/288]  
专题云南天文台_恒星物理研究组
推荐引用方式
GB/T 7714
Gu SH,Tan HS,Wang XB,et al. Surface Map of the RS CVn-type Star UX Arietis[C]. 见:the 219th symposium of the International Astronomical Union held during the IAU General Assembly XXV. Sydney, Australia. 2003-07-21.http://adsabs.harvard.edu/abs/2004IAUS..219..873G.

入库方式: OAI收割

来源:云南天文台

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