THE PHYSICAL PROPERTIES OF RED SUPERGIANTS
The "observed" location of red supergiants in the HRD has been at variance with the evolutionary tracks for many years, but the new generation of MARCS stellar atmosphere models has led to improved determinations of their physical properties, and much better agreement with stellar evolutionary theor...
Tallennettuna:
| Julkaisussa: | Revista Mexicana de Astronomía y Astrofísica |
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| Päätekijät: | , , , , , |
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
Universidad Nacional Autónoma de México
2008
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| Aiheet: | |
| Linkit: | https://www.redalyc.org/articulo.oa?id=57116159009 |
| Tagit: |
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