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Non-thermal radio emission from Wolf-Rayet stars

Published online by Cambridge University Press:  25 May 2016

Jessica M. Chapman ,
Claus Leitherer  and
Bärbel Koribalski
Jessica M. Chapman
Affiliation:
Anglo-Australian Observatory, PO Box 296, Epping, NSW 2121, Australia Australia Telescope National Facility, PO Box 76, Epping, NSW 2121, Australia
Claus Leitherer
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
Bärbel Koribalski
Affiliation:
Australia Telescope National Facility, PO Box 76, Epping, NSW 2121, Australia

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We have used the Australia Telescope Compact Array to search for radio continuum emission at λ 3, 6, 13 and 20 cm from a distance-limited sample of 36 southern Wolf-Rayet stars within 3 kpc of the Sun. The observations were taken between 1994 and 1997. Radio continuum emission has been detected from 16 sources at 3 cm. Of these 11 sources were detected at 6 cm, seven sources were detected at 13 cm and 2 sources were detected at 20 cm (Chapman et al. 1999).

Type
Part 1. Basic observational properties of Wolf-Rayet stars and other hot massive stars
Information
Symposium - International Astronomical Union , Volume 193: Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies , 1999 , pp. 59 - 60
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Chapman, J.M., Leitherer, C., Koribalski, B., Bouter, R., Storey, M. 1999 ApJ in press Google Scholar
Drissen, L., Robert, C., Moffat, A.F.J. 1992, ApJ 386, 288 CrossRefGoogle Scholar
Eichler, D., Usov, V. 1993, ApJ 402, 271 Google Scholar
Shara, M.M., Moffat, A.F.J., Smith, L.F., Potter, M. 1991, AJ 102, 716 CrossRefGoogle Scholar