No CrossRef data available.
Article contents
Superbubble Metallicities and X-ray Luminosities
Published online by Cambridge University Press: 03 August 2017
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 show that X-ray emission and dynamical properties of superbubbles around OB associations are affected by metal ejection from the enclosed Type II supernovae (SNe). The SN and massive star yields may significantly change the superbubble interior metallicity and enhance its X-ray luminosity.
- Type
- Part 3. Super Star Clusters and Associations
- Information
- Symposium - International Astronomical Union , Volume 207: Extragalactic Star Clusters , 2002 , pp. 459 - 460
- Copyright
- Copyright © Astronomical Society of the Pacific 2002
References
Silich, S.A., Tenorio-Tagle, G., Terlevich, R., Terlevich, E., & Netzer, H.
2001, MNRAS, 324, 191
Google Scholar
You have
Access