Long-term optical spectral observations of the Be/X-ray binary LSI+61 degrees 303: evidence of H alpha emission associated with the neutron star
Liu, QZ; Hang, HR; Wu, GJ; Chang, J; Zhu, ZX
刊名ASTRONOMY & ASTROPHYSICS
2000-07-01
卷号359期号:2页码:646-650
关键词stars : binaries : close stars : emission-line, Be stars : individual : LSI+61 degrees 303 X-rays : stars
ISSN号0004-6361
英文摘要We present the optical spectra of the periodic radio star LSI +61 degrees 303 with intermediate dispersion. The H alpha emission line profile and its variation an analyzed. Variability in LSI +61 degrees 303 is observed on different timescales. During our observations the equivalent width (EW) of H alpha line showed long-term variability that is likely to be associated with the 4-year period. We suggest that the long-term variability is connected to the intrinsic behaviour of the Be star.
学科主题Astronomy & Astrophysics
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]LSI +61-DEGREES-303 ; RADIO ; VARIABILITY ; MODULATION ; PERIODICITY
收录类别SCI
语种英语
WOS记录号WOS:000088587000029
公开日期2013-02-01
内容类型期刊论文
源URL[http://libir.pmo.ac.cn/handle/332002/8282]  
专题紫金山天文台_宇宙伽马暴、中子星及相关物理研究团组
作者单位1.Purple Mt Observ, Nanjing 210008, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100864, Peoples R China
3.Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands
4.Yunnan Observ, Kunming 650011, Peoples R China
推荐引用方式
GB/T 7714
Liu, QZ,Hang, HR,Wu, GJ,et al. Long-term optical spectral observations of the Be/X-ray binary LSI+61 degrees 303: evidence of H alpha emission associated with the neutron star[J]. ASTRONOMY & ASTROPHYSICS,2000,359(2):646-650.
APA Liu, QZ,Hang, HR,Wu, GJ,Chang, J,&Zhu, ZX.(2000).Long-term optical spectral observations of the Be/X-ray binary LSI+61 degrees 303: evidence of H alpha emission associated with the neutron star.ASTRONOMY & ASTROPHYSICS,359(2),646-650.
MLA Liu, QZ,et al."Long-term optical spectral observations of the Be/X-ray binary LSI+61 degrees 303: evidence of H alpha emission associated with the neutron star".ASTRONOMY & ASTROPHYSICS 359.2(2000):646-650.
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