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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 | Affiliation: | 1 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 | Abstract: | Long 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 | Services: | Forum | Review | PDF | Favorites |
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