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New Radio and Optical Data for GRO J1655–40

Published online by Cambridge University Press:  12 April 2016

Richard W. Hunstead
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia
Kinwah Wu
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia
Duncan Campbell-Wilson
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia

Abstract

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MOST 843 MHz flux densities are presented for the May 1996 outburst from GRO J1655—40. A deep radio image of the field reveals extended emission regions which may be associated with the radio jets. The optical spectrum during the 1994 outburst shows remarkable similarities to that of a Wolf-Rayet WN star.

Type
Part 2. Black Hole Transient Sources
Copyright
Copyright © Astronomical Society of the Pacific 1997

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