Long-duration neutron star X-ray transients in quiescence: the Chandra observation of KS 1731-260

dc.creatorWijnands, Rudy
dc.date2001-07-31
dc.date.accessioned2026-07-07T01:59:30Z
dc.date.available2026-07-07T01:59:30Z
dc.descriptionI will briefly discuss the implications of the recent quiescent Chandra observation of the long-duration neutron star transient KS 1731-260 (Wijnands et al. 2001a) on models for quiescent systems other than the Brown et al. (1998) cooling neutron star model. However, the Chandra results are not very constraining; for those models to be consistent with the data, one only has to assume that the system parameters of KS 1731-260 (e.g., the neutron star spin rate and magnetic field properties; orbital parameters) are very similar to those of the other systems. I will also discuss the available quiescent data of other long-duration neutron star transients in the context of the Brown et al. (1998) model.
dc.descriptionTo appear in "The High Energy Universe at Sharp Focus: Chandra Science", proceedings of the 113th Meeting of the Astronomical Society of the Pacific. 16-18 July 2001, St. Paul, MN
dc.identifierhttps://arxiv.org/abs/astro-ph/0107600
dc.identifierhttp://arxiv.org/abs/astro-ph/0107600
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3139
dc.subjectAstrophysics
dc.titleLong-duration neutron star X-ray transients in quiescence: the Chandra observation of KS 1731-260
dc.typetext

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