No CrossRef data available.
Article contents
ASCA observation of Henize 2-10
Published online by Cambridge University Press: 25 May 2016
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.
We present results of X-ray spectroscopy of the prototypical Wolf-Rayet galaxy Henize 2–10 with ASCA. We find that the X-ray spectrum is best described by a model with soft (kT ≃ 0.7 keV) and hard (kT ≃ 3.9 keV) components. The soft component is attributed to the hot gas associated with the superwind, and the hard component with a collection of the young sources (young SNRs and HMXBs) associated with the starburst.
- Type
- Part 5. Wolf-Rayet stars and other massive stars in starburst galaxies: the case of Wolf-Rayet galaxies (integrated spectra)
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 1999
References
Dickow, R., Hensler, G., Junkes, N.
1996, in: Kunth, D., Guiderdoni, B., Heydari-Malayeri, M. & Thuan, Trinh Xuan (eds.), The Interplay Between Massive Star Formation in the ISM and Galaxy Evolution (Gif-sur-Yvette: Editions Frontières), p. 583
Google Scholar
Kobulnicky, H.A., Dickey, J.M., Sargent, A.I., Hogg, D.E., Conti, P.S.
1995, AJ
110, 116
Google Scholar