Rauscher, T. and Heger, A. and Hoffman, R. D. and Woosley, S. E.. (2001) Nucleosynthesis in massive stars revisited. Nuclear physics. A, Nuclear and hadronic physics, Vol. 688, H. 1-2 , S. 193C-196C.
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Official URL: http://edoc.unibas.ch/dok/A5839313
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Abstract
We have performed the first calculations to follow the evolution of all stable nuclei and their radioactive progenitors in a finely-zoned stellar model computed from the onset of central hydrogen burning through explosion as a Type II supernova. Calculations were done for 15 M-circle dot, 20 M-circle dot, and 25 M-circle dot Pop I stars using the most recently available set of experimental and theoretical nuclear data, revised opacity tables, and taking into account mass loss due to stellar winds. Here results are presented for one 15 M-circle dot model.
| Faculties and Departments: | 05 Faculty of Science > Departement Physik > Former Organization Units Physics > Theoretische Physik Astrophysik (Thielemann) |
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| UniBasel Contributors: | Rauscher, Thomas |
| Item Type: | Article, refereed |
| Article Subtype: | Research Article |
| Publisher: | North Holland |
| ISSN: | 0375-9474 |
| Note: | Publication type according to Uni Basel Research Database: Journal article |
| Identification Number: |
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| Last Modified: | 14 Sep 2012 07:18 |
| Deposited On: | 14 Sep 2012 06:44 |
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