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Radio Properties of the X-Ray Binary GX 339–4

Published online by Cambridge University Press:  12 April 2016

R. K. Sood ,
D. Campbell-Wilson ,
Ph. Durouchoux ,
S. Corbel ,
R. Fender ,
R. Spencer ,
M. A. Nowak  and
A. K. Tzioumis
R. K. Sood
Affiliation:
Australian Defence Force Academy, UNSW, Canberra, Australia
D. Campbell-Wilson
Affiliation:
School of Physics, University of Sydney, Sydney, Australia
Ph. Durouchoux
Affiliation:
C.E. Saclay, DAPNIA, Service d’Astrophysique, France
S. Corbel
Affiliation:
C.E. Saclay, DAPNIA, Service d’Astrophysique, France
R. Fender
Affiliation:
Astronomy Centre, University of Sussex, Brighton, UK
R. Spencer
Affiliation:
University of Manchester, Jodrell Bank, Cheshire, UK
M. A. Nowak
Affiliation:
JILA, Colorado, USA
A. K. Tzioumis
Affiliation:
Australia Telescope National Facility, Epping, Australia

Abstract

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GX 339–4 has been monitored over a period of two and a half years with MOST and ATCA to investigate the flux variations and spatial structure of its radio emission. The data are summarized and discussed.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 349 - 350
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

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