the x-ray binary ks 1731{260: possible analogy with her x-1

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ID: 200728
2014
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Abstract
The X-ray binary with the neutron star (NS), KS 1731-260, displays superorbital cycle similar to that in Her X-1. The accretion disk had the memory of the cycle-length even when this modulation sometimes disappeared in the main outburst of KS 1731-260, and during anomalous low state in Her X-1. The disk still existed during such seasons. Although irradiation of the disk by X-rays is a viable explanation for the disk precession and warping (see model of Foulkes et al.), the mechanisms which give rise to the observed X-ray modulation are quite dierent for each of these systems. Variable absorption can explain this cycle only in Her X-1. We propose a variable mass accretion rate onto the NS in KS 1731-260 due to a highly variable impact of the inflowing mass stream with the changing phase of the cycle.
Reference Key
imon2014actathe Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors ;Vojtěch Šimon
Journal BMC Bioinformatics
Year 2014
DOI
10.14311/APP.2014.01.0246
URL
https://ojs.cvut.cz/ojs/index.php/APP/article/view/2403
Keywords
engineering (general) civil engineering (general)

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