期刊
NEW ASTRONOMY
卷 9, 期 4, 页码 249-264出版社
ELSEVIER
DOI: 10.1016/j.newast.2003.11.002
关键词
accretion : accretion disks; X-rays : binaries
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. (C) 2003 Elsevier B.V. All rights reserved.
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