SIMBAD references

2004NewA....9..249B - New Astronomy, 9, 249-264 (2004/May-0)

"Soft X-ray transient" outbursts which are not soft.

BROCKSOPP C., BANDYOPADHYAY R.M. and FENDER R.P.

Abstract (from CDS):

We have accumulated multiwavelength (X-ray, optical, radio) lightcurves for the eight black hole X-ray binaries which have been observed to enter a supposed `soft X-ray transient' outburst, but remained in the low/hard state throughout the outburst. Comparison of the lightcurve morphologies, spectral behaviour, properties of the quasi-periodic oscillations and the radio jet provides the first study of such objects as a sub-class of X-ray transients. However, rather than assuming that these hard state X-ray transients are different from the `canonical' soft X-ray transient, we prefer to consider the possibility that new analysis of both soft and hard state X-ray transients in a spectral context will provide a model capable of explaining the outburst mechanisms of (almost) all black hole X-ray binaries.

Abstract Copyright:

Journal keyword(s): Accretion: accretion disks - X-rays: binaries

Simbad objects: 16

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2021.03.04-22:28:25

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