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 language | English |
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Pages (from-to) | 659-663 |
Journal | Astronomy and Astrophysics |
Volume | 409 |
DOIs | |
Publication status | Published - 2003 |
Keywords
- . accretion, accretion disks
- globular clusters: individual: Terzan 6
- – X-rays: binaries
- X-rays: bursts
- X-rays: individuals: GRS 1747-312