A peculiar type-I X-ray burst from GRS 1747-312
Publication date
2003
Authors
in 't Zand, J.J.M.
Strohmayer, T.E.
Markwardt, C.B.
Swank, J.
Editors
Advisors
Supervisors
Document Type
Article
Metadata
Show full item recordCollections
License
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