First stars evolution and nucleosynthesis
The first stars in the universe were massive and luminous with typical masses M ≥ 100M . Metal-free stars have unique physical character- istics and exhibit high effective temperatures and small radii. These so called Population III stars were responsible for the initial enrichment of the intergalac...
Uloženo v:
| Vydáno v: | Revista Mexicana de Física |
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| Hlavní autoři: | , , |
| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
Sociedad Mexicana de Física A.C.
2007
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| Témata: | |
| On-line přístup: | https://www.redalyc.org/articulo.oa?id=57028300009 |
| Tagy: |
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