No CrossRef data available.
Article contents
Iron Abundance Discrepancy in Ellipticals after ASCA
Published online by Cambridge University Press: 25 May 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.
The chemical composition of the ISM is expected to reflect the average composition of the stellar component as established at the time of its formation, then further enriched by SN's of Type Ia that are known to currently explode in elliptical galaxies. Renzini et al. (1993) estimate the expected iron abundance in the hot ISM of elliptical galaxies to range from a minimum of ∼ 2 times solar, to perhaps as much as ∼ 5 times solar or more, depending on the adopted SNIa's rate.
- Type
- The Interstellar Medium
- Information
- Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 139 - 142
- Copyright
- Copyright © Kluwer 1996
References
Arimoto, N., Matsushita, K., Ishimaru, Y., Ohashi, T., & Renzini, A., 1995, in preparation
Google Scholar
Fabian, A.C., Thomas, P.A., Fall, S.M., and White, R.E. III
1986, MNRAS, 221, 1049
CrossRefGoogle Scholar
You have
Access