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

J.J.M. in 't Zand, T.E. Strohmayer, C.B. Markwardt, J. Swank

Research output: Contribution to journalArticleAcademicpeer-review

Abstract

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.
Original languageEnglish
Pages (from-to)659-663
JournalAstronomy and Astrophysics
Volume409
DOIs
Publication statusPublished - 2003

Keywords

  • . accretion, accretion disks
  • globular clusters: individual: Terzan 6
  • – X-rays: binaries
  • X-rays: bursts
  • X-rays: individuals: GRS 1747-312

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