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...
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| 出版年: | Revista Mexicana de Astronomía y Astrofísica |
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| 主要な著者: | , , , , , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
Universidad Nacional Autónoma de México
2008
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| 主題: | |
| オンライン･アクセス: | https://www.redalyc.org/articulo.oa?id=57116159009 |
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