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The Global X-Ray Burst Behaviour of KS 1731-260

Published online by Cambridge University Press:  22 February 2018

R. Cornelisse
R. Cornelisse*
Affiliation:
School of Physics and Astronomy, Southampton University, SO17 1BJ, UK (cornelis@astro.soton.ac.uk)

Abstract

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An overview is given of the type I X-ray burst properties of the transient KS 1731-260. These characteristics appear to be proto-typical for all type I X-ray bursters, and stable helium burning occuring at high mass accretion rates could explain them.

Resumen

Resumen

Se presenta, una revisión de las propiedades de los brotes de rayos X de tipo I del sistema transitorio KS1731-260. Estas características parecen ser prototípicas para todos los brotes de rayos X de tipo I y podrían explicarse por la, quema estable de helio que ocurre a altas tasas de acreción de masa.

Keywords

AccretionAccretion Discs — Stars: Neutron — X-Rays: Bursts
Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 10 - 11
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

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