No CrossRef data available.
Article contents
On the Progenitors of Type Ia Supernovae
Published online by Cambridge University Press: 19 July 2016
Extract
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.
Supersoft X-ray sources (hereafter SSS) are a class of luminous (bolometric luminosity ~ 1037 − 1038 erg s−1) objects with a characteristic radiation temperature of 30 to 60 eV (Hasinger 1994; Kahabka & Trümper 1996). The most popular model for SSS is that they are massive white dwarfs steadily burning nuclear fuel accreted from a more massive binary companion at a rate near or above the Eddington limit (van den Heuvel et al. 1992).
- Type
- Conference Papers in order of Presentation
- Information
- Symposium - International Astronomical Union , Volume 187: Cosmic Chemical Evolution , 2002 , pp. 103 - 108
- Copyright
- Copyright © 2002
References
Cowley, A. P. et al. (1996) in
IAU Symp. 165, Compact Stars in Binaries
, eds. van Paradijs, J., van den Heuvel, E. P. J. & Kuulkers, E. (Dordrecht: Kluwer), 439.Google Scholar
Di Stefano, R. and Nelson, N. A. (1996) in
Supersoft X-ray Sources
, ed. Greiner, J. (Berlin: Springer), 3.CrossRefGoogle Scholar
Kahabka, P and Trümper, J. (1996) in
IAU Symp. 165, Compact Stars in Binaries
, eds. van Paradijs, J., van den Heuvel, E. P. J. & Kuulkers, E. (Dordrecht: Kluwer), 425.CrossRefGoogle Scholar
You have
Access