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Chinese Academy of Sciences Institutional Repositories Grid
Distribution and evolution of starspots on the RS CVn binary II Pegasi in 2004

文献类型:期刊论文

作者Xiang Y(项越)1,2,3; Gu SH(顾盛宏)1,2; Cameron, AC4; Barnes, JR5
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2014-03
卷号438期号:3页码:2307-2316
关键词stars: activity binaries: close stars: imaging stars: individual: II Peg starspots
ISSN号0035-8711
产权排序第一完成单位
通讯作者Xiang, Y (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China.
英文摘要We present Doppler images of RS CVn-type binary II Peg based on two data sets obtained in 2004 February and November. In order to improve signal-to-noise ratio and reliability, we apply least-squares deconvolution technique to calculate average profiles from 2032 photospheric absorption lines. Both of the resulting surface images show a wide latitude distribution of starspots. Most spots are concentrated at a high-latitude belt above 60 degrees and a low-latitude belt near equator. The starspots evolved dramatically between two observing runs, which may indicate shorter time-scale evolution in this epoch, especially for low-latitude belt. There is no stable preferred active longitude that can be found in our images. We also find out a possible phenomenon that the intermediate-latitude spot migrated poleward and merged with the high-latitude spot to make it stronger, which may reveal a more complex behaviour of starspots on II Peg. A potential change of orbital ephemeris zero-point was detected. This may imply an orbital period change of II Peg like other active close binaries.
WOS标题词Science & Technology ; Physical Sciences
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]ORBITAL PERIOD MODULATION ; STELLAR SURFACE-STRUCTURE ; CANUM-VENATICORUM ; ACTIVE STARS ; DIFFERENTIAL ROTATION ; DOPPLER IMAGES ; SPOT ACTIVITY ; V711 TAURI ; HR 1099 ; ACTIVITY CYCLE
收录类别SCI
原文出处http://mnras.oxfordjournals.org/content/438/3/2307
语种英语
WOS记录号WOS:000331877000024
公开日期2016-05-03
源URL[http://ir.ynao.ac.cn/handle/114a53/6801]  
专题云南天文台_系外行星研究组
云南天文台_中国科学院天体结构与演化重点实验室
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China
2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China
3.University of Chinese Academy of Sciences, Beijing 100049, China
4.School of Physics and Astronomy, University of St Andrews, Fife KY16 9SS, UK
5.Centre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield, Hertfordshire AL10 9AB, UK
推荐引用方式
GB/T 7714
Xiang Y,Gu SH,Cameron, AC,et al. Distribution and evolution of starspots on the RS CVn binary II Pegasi in 2004[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2014,438(3):2307-2316.
APA Xiang Y,Gu SH,Cameron, AC,&Barnes, JR.(2014).Distribution and evolution of starspots on the RS CVn binary II Pegasi in 2004.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,438(3),2307-2316.
MLA Xiang Y,et al."Distribution and evolution of starspots on the RS CVn binary II Pegasi in 2004".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 438.3(2014):2307-2316.

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