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Observations of light elements in massive stars
| Content Provider | Scilit |
|---|---|
| Author | Kaufer, A. |
| Copyright Year | 2009 |
| Description | Observations of light elements in hot massive stars are limited to few transitions of boron in the satellite-ultraviolet; lithium and beryllium are not observable at all. But because of its high sensitivity to the effects of rotational mixing, boron abundance determinations in massive stars have excelled as the definite test for evolutionary models with rotation. In this paper the observational evidence for rotational mixing in massive stars is reviewed and alternative interpretations are discussed. |
| Related Links | https://www.cambridge.org/core/services/aop-cambridge-core/content/view/CA2267A6FD2B6E10FEE9093F2188BD97/S1743921310004291a.pdf/div-class-title-observations-of-light-elements-in-massive-stars-div.pdf |
| Ending Page | 324 |
| Page Count | 8 |
| Starting Page | 317 |
| ISSN | 17439213 |
| e-ISSN | 17439221 |
| DOI | 10.1017/s1743921310004291 |
| Journal | Proceedings of the International Astronomical Union |
| Issue Number | S268 |
| Volume Number | 5 |
| Language | English |
| Publisher | Cambridge University Press (CUP) |
| Publisher Date | 2009-11-01 |
| Access Restriction | Open |
| Subject Keyword | Proceedings of the International Astronomical Union Astronomy and Astrophysics Nuclear Physics Abundances |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |
