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19 April 2024 |
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X-Ray Jet Emission from the Black Hole X-Ray Binary XTE J1550-564 with Chandra in 2000 | | John A. Tomsick
; Stephane Corbel
; Rob Fender
; Jon M. Miller
; Jerome A. Orosz
; Tasso Tzioumis
; Rudy Wijnands
; Philip Kaaret
; | | Date: |
17 Oct 2002 | | Journal: | Astrophys.J. 582 (2003) 933-944 | | Subject: | astro-ph | | Affiliation: | CASS/UCSD), Stephane Corbel (Universite Paris VII and CEA Saclay), Rob Fender (University of Amsterdam), Jon M. Miller (MIT), Jerome A. Orosz (Utrecht University), Tasso Tzioumis (ATNF), Rudy Wijnands (MIT and Chandra Fellow), Philip Kaaret (Harvard-Sm | | Abstract: | We have discovered an X-ray jet due to material ejected from the black hole X-ray transient XTE J1550-564. The discovery was first reported by Corbel et al. (Science, 298, 196 and astro-ph/0210224), and here, we present an analysis of the three Chandra observations made between 2000 June and 2000 September. For these observations, a source is present that moves in an eastward direction away from the point source associated with the compact object. The separation between the new source and the compact object changes from 21.3 arcseconds in June to 23.4 arcseconds in September, implying a proper motion of 21.2 +/- 7.2 mas/day, a projected separation of 0.31-0.85 pc and an apparent jet velocity between 0.34 +/- 0.12 and 0.93 +/- 0.32 times the speed of light for a source distance range of d = 2.8-7.6 kpc. These observations represent the first time that an X-ray jet proper motion measurement has been obtained for any accretion powered Galactic or extra-galactic source. While this work deals with the jet to the east of the compact object, the western jet has also been detected in the X-ray and radio bands. The most likely scenario is that the eastern jet is the approaching jet and that the jet material was ejected from the black hole in 1998. Along with a 1998 VLBI proper motion measurement, the Chandra proper motion indicates that the eastern jet decelerated between 1998 and 2000. We present results on the morphology and energy spectrum of the jet. We cannot definitively determine the X-ray emission mechanism, but a synchrotron origin is viable and may provide the simplest explanation for the observations. | | Source: | arXiv, astro-ph/0210399 | | Services: | Forum | Review | PDF | Favorites | |
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