A peculiar type-I X-ray burst from GRS 1747-312

被引:16
作者
in 't Zand, JJM
Strohmayer, TE
Markwardt, CB
Swank, J
机构
[1] SRON, Natl Inst Space Res, NL-3584 CA Utrecht, Netherlands
[2] Univ Utrecht, Astron Inst, NL-3508 TA Utrecht, Netherlands
[3] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[4] Univ Maryland, Dept Astron, College Pk, MD 20742 USA
关键词
accretion; accretion disks; globular clusters : individual : Terzan 6; X-rays : binaries; X-rays : bursts; X-rays : individuals : GRS 1747-312;
D O I
10.1051/0004-6361:20031042
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the serendipitous detection with the Rossi X-ray Timing Explorer of a long and peculiar X-ray burst whose position is consistent with one known X-ray burster (GRS 1747-312) and which occurred when that source was otherwise quiescent. The peculiar feature concerns a strong radius expansion of the neutron star photosphere, which occurred not within a few seconds from the start of the burst, as is standard in radius-expansion bursts, but 20 s later. This suggests that two different layers of the neutron star may have undergone thermonuclear runaways: a hydrogen-rich and a hydrogen-poor layer. The reason for the delay may be related to the source being otherwise quiescent.
引用
收藏
页码:659 / 663
页数:5
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