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Artículo de revista

The Thermonuclear X-Ray Bursts of 4U 1730-22

Peter Bult ... [et al.].

Serie: Trabajos publicados del IAR ; no. 1719

Resumen: 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 173-22 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 1-2 s rise times and a photospheric radius expansion phase, while the weak bursts showed a slower [aprox.]5 s rise with a tendency for concave shapes. From the photospheric radius expansion flux, we estimate the source distance at 6.9 ± 0.2 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

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The Astrophysical Journal ISSN 0004-637X — Vol. 940, (2022), p. 81
 
Registro 001936 · Modificado: 03/01/2023

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