中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The last three outbursts of H1743-322 observed by RXTE in its latest service phase

文献类型:期刊论文

作者Zhou, JN; Liu, QZ; Chen YP(陈玉鹏); Chen, YP; Li, J; Qu, JL; Zhang, S; Gao, HQ; Zhang, Z; Li J(李剑)
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2013
卷号431期号:3页码:2285-2293
关键词X-rays: binaries X-rays: individual: IGR J17464-3213 X-rays: individual: H1743-322 X-rays: stars
英文摘要After 2010, three outbursts of H1743-322 were detected by RXTE. We have carried out timing and spectral analysis of the data, emphasizing on the two with relatively complete evolution history presented in the RXTE/Proportional Counter Array observations. We then constitute an enlarged outburst sample for H1743-322 which allows us to investigate the spectral transitions in more details. We find that the spectral transitions to high-soft state constrain a region for four outbursts in hardness-intensity diagram. An extension of the region locates in the vicinity of the failed outburst in 2008, and excludes it from a successful group. We therefore suggest that the failed outburst in 2008 may present the first almost successful outburst sample, which is important for modelling the outburst, especially upon the conditions required for transition to high-soft state.
学科主题Astronomy & Astrophysics
收录类别SCI
WOS记录号WOS:000318347500021
公开日期2016-05-03
源URL[http://ir.ihep.ac.cn/handle/311005/224197]  
专题高能物理研究所_粒子天体物理中心
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GB/T 7714
Zhou, JN,Liu, QZ,Chen YP,et al. The last three outbursts of H1743-322 observed by RXTE in its latest service phase[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2013,431(3):2285-2293.
APA Zhou, JN.,Liu, QZ.,陈玉鹏.,Chen, YP.,Li, J.,...&Zhang Z.(2013).The last three outbursts of H1743-322 observed by RXTE in its latest service phase.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,431(3),2285-2293.
MLA Zhou, JN,et al."The last three outbursts of H1743-322 observed by RXTE in its latest service phase".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 431.3(2013):2285-2293.

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来源:高能物理研究所

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