中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
An additional H alpha emission component in LSI+61 degrees 303: Further evidence for the H alpha emission related to the neutron star

文献类型:期刊论文

作者Liu, QZ; Yan, JZ
刊名NEW ASTRONOMY
出版日期2005-11-01
卷号11期号:2页码:130-137
关键词stars individual LSI+61 degrees 303-X-rays stars-stars emission-line Be stars binaries close
ISSN号1384-1076
英文摘要A long-term program has been established since 1992 to monitor more than a dozen of observable X-ray binaries. We present the long-term spectroscopic results of the Be/X-ray binary, LSI+61 degrees 303. The Hot emission line, usually observed as a double-peaked profile with a dominant red peak, varies noticeably during our program. While the blue peak of the Hot emission line decreases gradually, the red peak increases considerably in 2002 October observational run and remains relatively unchanged in 2004 September run. We attribute these variations to the asymmetric perturbation in the Be envelope. Finally, we report on the discovery of a two-component structure in the Ha emission line when close to the apastron. In addition to the original double-peaked Ha emission component, an additional emission component emerges at the center part of the emission line, which could originate in the accretion disc around the neutron star. (c) 2005 Elsevier B.V. All rights reserved.
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]LS-I +61-DEGREES-303 ; X-RAY BINARIES ; RADIO OBSERVATIONS ; LIGHT-CURVE ; I+61-DEGREES-303 ; &61-DEGREES-303 ; VARIABILITY ; PERIODICITY ; MODULATION ; JET
收录类别SCI
语种英语
WOS记录号WOS:000233303000005
公开日期2012-03-07
源URL[http://159.226.72.40/handle/332002/4178]  
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.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
推荐引用方式
GB/T 7714
Liu, QZ,Yan, JZ. An additional H alpha emission component in LSI+61 degrees 303: Further evidence for the H alpha emission related to the neutron star[J]. NEW ASTRONOMY,2005,11(2):130-137.
APA Liu, QZ,&Yan, JZ.(2005).An additional H alpha emission component in LSI+61 degrees 303: Further evidence for the H alpha emission related to the neutron star.NEW ASTRONOMY,11(2),130-137.
MLA Liu, QZ,et al."An additional H alpha emission component in LSI+61 degrees 303: Further evidence for the H alpha emission related to the neutron star".NEW ASTRONOMY 11.2(2005):130-137.

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来源:紫金山天文台

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