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

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.

Keywords

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

Citation

in 't Zand, J J M, Strohmayer, T E, Markwardt, C B & Swank, J 2003, 'A peculiar type-I X-ray burst from GRS 1747-312', Astronomy and Astrophysics, vol. 409, pp. 659-663. https://doi.org/10.1051/0004-6361:20031042