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Orbital period analyses for the CVs inside the period gap
Dai ZB(戴智斌); Qian SB(钱声帮); Dai ZB(戴智斌); Qian SB(钱声帮)
刊名Memorie della Societa Astronomica Italiana
2012
卷号83期号:1页码:614-618
关键词Stars: cataclysmic variables Stars : binaries : close
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英文摘要All 13 eclipse CVs inside period gap are investigated. Considering that most CVs inside period gap lack the enough data accumulation, We only choose five objects to make orbital period analysis including a prototype polar AM Her and pre-CVs HW Vir. Although AM Her is not an eclipsing CVs, the facts that its orbital period locates in the upper edge of gap and it has a stable timing system suggest that AM Her should be a significant object for the study of period gap. All orbital period analyses for the CVs inside period gap never indicates any secular evolution information, which may suggest that the CVs inside period gap have a different evolution end. Moreover, the complex O-Cs variations can be explained by the light trave-time effect. It means that there are many substellar objects surrounding the CVs.
学科主题天文学
收录类别其他
原文出处http://adsabs.harvard.edu/abs/2012MmSAI..83..614D
语种英语
内容类型期刊论文
源URL[http://ir.ynao.ac.cn/handle/114a53/5871]  
专题云南天文台_双星与变星研究组
云南天文台_中国科学院天体结构与演化重点实验室
推荐引用方式
GB/T 7714
Dai ZB,Qian SB,Dai ZB,et al. Orbital period analyses for the CVs inside the period gap[J]. Memorie della Societa Astronomica Italiana,2012,83(1):614-618.
APA 戴智斌,钱声帮,Dai ZB,&Qian SB.(2012).Orbital period analyses for the CVs inside the period gap.Memorie della Societa Astronomica Italiana,83(1),614-618.
MLA 戴智斌,et al."Orbital period analyses for the CVs inside the period gap".Memorie della Societa Astronomica Italiana 83.1(2012):614-618.
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