Abstract
The discovery of the association between relativistic radio jets and X-ray events in GRS 1915+105 (Mirabel and Rodriguez, 1994) and GRO J1655-40 showed that strong radio flares (Harmon et al, 1994) in general, and jet ejection (Hjellming and Rupen, 1994) in particular, could be identified with features in hard X-ray events. This has caused us to re-think the interpretation of the radio events in X-ray transients, and has made multi-wavelength observations even more important. In this paper the focus is on the connection between X-ray and radio events as seen since 1994 in GRS 1915+105, GRO J1655-40, GRO J1719-24, GRO J1739-278, Cyg X-3, Cyg X-l, and Sco X-l.KeywordsBlack HoleRadio EmissionProper MotionAdvection Dominate Accretion FlowRelated OutflowThese keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
