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TYPE-I X-RAY BURSTS REVEAL A FAST CO-EVOLVING BEHAVIOR OF THE CORONA IN AN X-RAY BINARY
Chen YP(陈玉鹏); Zhang S(张澍); Zhang SN(张双南); Li J(李剑); 王建民;Chen, YP; Zhang, S; Zhang, SN; Li, J; Wang, JM
2012
发表期刊ASTROPHYSICAL JOURNAL LETTERS
卷号752期号:2页码:L34
摘要The coronae in X-ray binaries (XRBs) still remain poorly understood, although they have been believed for a long time to play a key role in modeling the characteristic outbursts of XRBs. Type-I X-ray bursts, the thermonuclear flashes happening on the surface of a neutron star (NS), can be used as a probe to the innermost region of an NS XRB, where the corona is believed to be located very close to the NS. We report the discovery of a tiny life cycle of the corona that is promptly co-evolved with the type-I bursts superimposed on the outburst of the NS XRB IGR J17473-2721. This finding may serve as the first evidence of directly seeing the rapid disappearance and formation of a corona in an XRB with a cooling/heating timescale of less than a second, which can strongly constrain the accretion models in XRBs at work.
关键词stars: coronae stars: neutron X-rays: binaries X-rays: bursts X-rays: individual (IGR J17473-2721)
学科领域Astronomy & Astrophysics
DOI10.1088/2041-8205/752/2/L34
收录类别SCI
WOS记录号WOS:000305461600017
引用统计
被引频次:14[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ihep.ac.cn/handle/311005/224738
专题粒子天体物理中心
推荐引用方式
GB/T 7714
Chen YP,Zhang S,Zhang SN,et al. TYPE-I X-RAY BURSTS REVEAL A FAST CO-EVOLVING BEHAVIOR OF THE CORONA IN AN X-RAY BINARY[J]. ASTROPHYSICAL JOURNAL LETTERS,2012,752(2):L34.
APA 陈玉鹏.,张澍.,张双南.,李剑.,王建民;Chen, YP.,...&Wang, JM.(2012).TYPE-I X-RAY BURSTS REVEAL A FAST CO-EVOLVING BEHAVIOR OF THE CORONA IN AN X-RAY BINARY.ASTROPHYSICAL JOURNAL LETTERS,752(2),L34.
MLA 陈玉鹏,et al."TYPE-I X-RAY BURSTS REVEAL A FAST CO-EVOLVING BEHAVIOR OF THE CORONA IN AN X-RAY BINARY".ASTROPHYSICAL JOURNAL LETTERS 752.2(2012):L34.
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