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27 April 2024
 
  » arxiv » astro-ph/0407070

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Long term variability of Cygnus X-1, III. Radio-X-ray correlations
T. Gleissner ; J. Wilms ; G. G. Pooley ; M. A. Nowak ; K. Pottschmidt ; S. Markoff ; S. Heinz ; M. Klein-Wolt ; R. P. Fender ; R. Staubert ;
Date 3 Jul 2004
Journal Astron.Astrophys. 425 (2004) 1061-1068
Subject astro-ph
Affiliation1 and 2), G. G. Pooley , M. A. Nowak , K. Pottschmidt (5 and 6), S. Markoff , S. Heinz , M. Klein-Wolt , R. P. Fender , R. Staubert ( Univ. Tuebingen, Univ. Warwick, MRAO, MIT, MPE, ISDC, Univ. Amsterdam
AbstractLong time scale radio-X-ray correlations in black holes during the hard state have been found in many sources and there seems to emerge a universal underlying relationship which quantitatively describes this behavior. Although it would appear only natural to detect short term emission patterns in the X-ray and - with a certain time lag - in the radio, there has been little evidence for this up to now. The most prominent source for radio-X-ray correlations on short time scales (minutes) so far remains GRS 1915+105 where a single mass ejection could be detected successively in the X-ray, IR, and radio wavebands. We analyze a database of more than 4 years of simultaneous radio-X-ray data for Cygnus X-1 from the Ryle Telescope and RXTE PCA/HEXTE. We confirm the existence of a radio-X-ray correlation on long time scales, especially at hard energies. We show that apparent correlations on short time scales in the lightcurves of Cygnus X-1 are most likely the coincidental outcome of white noise statistics. Interpreting this result as a breakdown of radio-X-ray correlations on shorter time scales, this sets a limit to the speed of the jet.
Source arXiv, astro-ph/0407070
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