The last three outbursts of H1743-322 observed by RXTE in its latest service phase

CORC > 高能物理研究所 > 中国科学院高能物理研究所 > 粒子天体物理中心

	The last three outbursts of H1743-322 observed by RXTE in its latest service phase
	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
	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
内容类型	期刊论文
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
推荐引用方式 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.