Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-26T18:40:42.631Z Has data issue: false hasContentIssue false
  • English
  • Français

New Radio and Optical Data for GRO J1655–40

Published online by Cambridge University Press:  12 April 2016

Richard W. Hunstead ,
Kinwah Wu  and
Duncan Campbell-Wilson
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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 63 - 67
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Bailyn, C.D. et al. 1995, Nature, 374, 701.Google Scholar
Casares, J. et al. 1991, MNRAS, 250, 712.Google Scholar
Hamann, W.-R. et al. 1995, A&AS, 113, 459.Google Scholar
Hjellming, R.M. and Rupen, M.P. 1995, Nature, 375, 8 CrossRefGoogle Scholar
Hjellming, R.M. and Rupen, M.P. 1996, IAU Circ 6411.Google Scholar
Hunstead, R.W. et al. 1995, Compact Stars in Binaries, eds. van Paradijs, J. et al., Dordrecht: Kluwer, p.369 Google Scholar
Hunstead, R. and Campbell-Wilson, D. 1996, IAU Circ 6410.Google Scholar
van Kerkwijk, M.H. et al. 1992, Nature, 355, 703.CrossRefGoogle Scholar
Remillard, R. et al. 1996, IAU Circ 6393.Google Scholar
Robertson, J.G. 1991, Aust J Phys, 44, 729.CrossRefGoogle Scholar