中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Spectral variability of the massive X-ray binary LSI+65 degrees 010

文献类型:期刊论文

作者Liu, QZ; Hang, HR
刊名ASTRONOMY & ASTROPHYSICS
出版日期1999-10-01
卷号350期号:3页码:855-858
关键词line : profiles stars : individual : LSI+65 degrees 010 stars : supergiants X-rays : stars
英文摘要We present optical spectroscopic observations of the massive X-ray binary LSI +65 degrees 010, the optical counterpart to the X-ray transient 2S0114+65. Our data show a dramatic variability in 1992 and only a mild variability during 1993-1995. An increase by a factor more than three in the equivalent width of the H alpha emission line within four days is present in Nov. 1992. It is interesting to notice that changes have taken place only in the blue side on Nov. 4, 1992, when compared to similar spectrum taken one day before. We associate this phenomenon with the existence of an HII region around the neutron star. A double-peak profile is seen in the spectrum of Sept. 1994. If this double-peak profile is real, we suggest that such a profile may be explained by the emission line from an HII region around the neutron star, superposed on that from the stellar wind of the supergiant.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]OPTICAL COUNTERPART ; 2S 0114+650 ; SYSTEM ; 2S-0114+650
收录类别SCI
语种英语
WOS记录号WOS:000083801100023
源URL[http://libir.pmo.ac.cn/handle/332002/15989]  
专题紫金山天文台_空间目标与碎片观测研究基地
作者单位1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Nanjing 210008, Peoples R China
推荐引用方式
GB/T 7714
Liu, QZ,Hang, HR. Spectral variability of the massive X-ray binary LSI+65 degrees 010[J]. ASTRONOMY & ASTROPHYSICS,1999,350(3):855-858.
APA Liu, QZ,&Hang, HR.(1999).Spectral variability of the massive X-ray binary LSI+65 degrees 010.ASTRONOMY & ASTROPHYSICS,350(3),855-858.
MLA Liu, QZ,et al."Spectral variability of the massive X-ray binary LSI+65 degrees 010".ASTRONOMY & ASTROPHYSICS 350.3(1999):855-858.

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