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Neutron sources during shell C-burning in massive stars
| Content Provider | Scilit |
|---|---|
| Author | Pignatari, Marco Gallino, R. Baldovin, C. Herwig, F. |
| Copyright Year | 2005 |
| Description | We present a study of the s–process nucleosynthesis (weak s-process) occurring during convective core He–burning and convective shell Carbon–burning in a massive star of 25 M. We use an updated nuclear network for the various neutron sources and for all neutron captures and β-decay rates involved. Large uncertainties affect the final yields due to the present unsatisfactory knowledge of all neutron capture cross sections involved. |
| Related Links | https://www.cambridge.org/core/services/aop-cambridge-core/content/view/7B4365D641F8CBE0D5F4604AFB441446/S1743921305006320a.pdf/div-class-title-neutron-sources-during-shell-c-burning-in-massive-stars-div.pdf |
| Ending Page | 496 |
| Page Count | 2 |
| Starting Page | 495 |
| ISSN | 17439213 |
| e-ISSN | 17439221 |
| DOI | 10.1017/s1743921305006320 |
| Journal | Proceedings of the International Astronomical Union |
| Issue Number | S228 |
| Volume Number | 1 |
| Language | English |
| Publisher | Cambridge University Press (CUP) |
| Publisher Date | 2005-05-01 |
| Access Restriction | Open |
| Subject Keyword | Proceedings of the International Astronomical Union Nuclear Reactions Abundances |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |
