The thermonuclear X-ray bursts of 4U 1730-22
arXiv:2210.09079 · doi:10.3847/1538-4357/ac9b26
Abstract
We present observations of the historic transient 4U 1730-22 as observed with the Neutron Star Interior Composition Explorer (NICER). After remaining in quiescence since its 1972 discovery, this X-ray binary showed renewed outburst activity in 2021 and 2022. We observed 4U 1730-22 extensively with NICER, detecting a total of 17 thermonuclear X-ray bursts. From a spectroscopic analysis, we find that these X-ray bursts can be divided into a group of bright and weak bursts. All bright bursts showed second rise times and a photospheric radius expansion phase, while the weak bursts showed a slower second rise with a tendency for concave shapes. From the photospheric radius expansion flux, we estimate the source distance at kpc. We consider various interpretations for our observations and suggest that they may be explained if accreted material is burning stably at the stellar equator, and unstable ignition occurs at a range of higher latitudes.
13 pages, 6 figures, 2 tables. Accepted for publication in ApJ
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