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A relativistic jet from Cygnus X-1 in the low/hard X-ray state

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Stirling, A. M., Spencer, R. E., de La Force, C. J., Garrett, M. A., Fender, R. P., Ogley, R. N.·2001·Monthly Notices of the Royal Astronomical Society

Abstract

We present the detection of a radio-emitting jet from the black hole candidate and X-ray binary source Cygnus X-1. Evidence of a bright core with a slightly extended structure was found on milliarcsecond resolution observations with the Very Long Baseline Array (VLBA) at 15.4 GHz. Later observations with the VLBA [and including the phased-up, Very Large Array (VLA)] at 8.4 GHz show an extended jet-like feature extending to ∼ 15 mas from a core region, with an opening angle of < 2°. In addition, lower resolution MERLIN observations at 5 GHz show that the source has < 10 per cent linear polarization. The source was in the low/hard X-ray state during the observations, and the results confirm the existence of persistent radio emission from an unresolved core and a variable, relativistic (> 0.6c) jet during this state.

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Metadata

Authors
Stirling, A. M., Spencer, R. E., de La Force, C. J., Garrett, M. A., Fender, R. P., & Ogley, R. N.
Venue
Monthly Notices of the Royal Astronomical Society
Published
2001-11-11
Volume
327
Issue
4
Pages
1273-1278
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2009154954
Cited by
387
References
0
FWCI
11.40
Type
journal article
Language
en
Open access
bronze

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Stirling, A. M., Spencer, R. E., de La Force, C. J., Garrett, M. A., Fender, R. P., & Ogley, R. N. (2001). A relativistic jet from Cygnus X-1 in the low/hard X-ray state. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1046/j.1365-8711.2001.04821.x

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