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Imaging Relativistic Radio Jets and the X-ray-Radio Connection in X-ray Transients

Published online by Cambridge University Press:  12 April 2016

R. M. Hjellming
R. M. Hjellming*
Affiliation:
National Radio Astronomy Observatory, Socorro, NM 87801

Abstract

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The superluminal radio jets produced by GRO J1655–40 during a series of X-ray outbursts in 1994 were the first indications of a delayed form of relativistic outflows from black hole accretion disk environments. In this paper we review the relation between the radio jets and changes in the X-ray environment for the 1994 events in GRO J1655–40 and compare this behavior with similar X-ray-radio correlations that have since been found in GRS 1716–249, GRS 1739–278, and the 1996 recurrence of another correlated event in GRO 1655–40. We also discuss newly found radio-X-ray correlations in a galactic X-ray binary, Cyg X–3.

Type
Part 2. Black Hole Transient Sources
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 53 - 62
Copyright
Copyright © Astronomical Society of the Pacific 1997

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