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An X-ray survey of Wolf-Rayet galaxies

Published online by Cambridge University Press:  25 May 2016

Ian R. Stevens
Affiliation:
The University of Birmingham, Edgbaston, Birmingham B15 2TT, UK
David K. Strickland
Affiliation:
The Johns Hopkins University, Baltimore, MD 21218-2686, USA

Abstract

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We report on an ongoing survey of the X-ray properties of Wolf-Rayet galaxies. The current sample now has 14 detections, as well as a number of upper-limits. WR galaxies have soft thermal X-ray spectra with properties consistent with an origin from superbubbles in a young starburst.

Type
Part 5. Wolf-Rayet stars and other massive stars in starburst galaxies: the case of Wolf-Rayet galaxies (integrated spectra)
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Kobulnicky, H.A., Skillman, E.D. 1997, ApJ 489, 636 CrossRefGoogle Scholar
Read, A.M., Ponman, T.J., Strickland, D.K. 1997, MNRAS 286, 626 Google Scholar
Stevens, I.R., Strickland, D.K. 1998a, MNRAS 294, 523 Google Scholar
Stevens, I.R., Strickland, D.K. 1998b, MNRAS 301, 215 CrossRefGoogle Scholar