Panel discussion section H
Dworetsky: In the blue metal poor stars shown by you (from C. Sneden) you had a lot of Pb. Were there any signs of Hg, Mn, or Y, typical signatures of diffusion? Or is nuclear processing a sufficient explanation without diffusion?To search for other articles by the author(s) go to: http://adsabs.har...
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| Veröffentlicht in: | Proceedings of the International Astronomical Union 2004-07, Vol.2004 (IAUS224), p.419-421 |
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| Format: | Artikel |
| Sprache: | eng |
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| Online-Zugang: | Volltext |
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| Zusammenfassung: | Dworetsky: In the blue metal poor stars shown by you (from C. Sneden) you had a lot of Pb. Were there any signs of Hg, Mn, or Y, typical signatures of diffusion? Or is nuclear processing a sufficient explanation without diffusion?To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html |
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| ISSN: | 1743-9213 1743-9221 |
| DOI: | 10.1017/S1743921304004831 |