| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10694518 | Advances in Space Research | 2005 | 5 Pages |
Abstract
A detailed analysis of the element abundance ratios provides evidence that the SN Ia yields in the central cluster galaxies are more rich in intermediate mass elements, like Si and S, compared to the SN Ia models used to explain the heavy element enrichment in our Galaxy.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
H. Böhringer, K. Matsushita, A. Finoguenov, Y. Xue, E. Churazov,