Multiwavelength observations of the black hole candidate Swift J1753.5-0127

Details Multiwavelength observations of the black hole candidate Swift J1753.5-0127 Multiwavelength observations of the black hole candidate Swift J1753.5-0127

2008-03-12

arxiv.org/abs/0803.1735v1

AIP Conf.Proc.1010:103-106,2008

Astronomy and Astrophysics

Astrophysics

4 pages, 1 figure; to be published in proceedings of "A Population Explosion: The Nature and Evolution of X-ray Binaries in Di

Scientific paper

10.1063/1.2945015

We present preliminary results from the analysis of simultaneous multiwavelength observations of the black hole candidate Swift J1753.5-0127. The source is still continuing its outburst started in May 2005, never leaving the Low/Hard State. In the X-ray energy spectra we confirm evidence for a thermal component at a very low luminosity possibly extending close to but not at the innermost stable orbit. This is unusual for black hole candidates in the Low/Hard State. Furthermore, we confirm that its radio emission is significantly fainter than expected from the relation observed in other black hole candidates between the observed radio/X-ray fluxes.

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