HIGH-CONTRAST COMPANIONS AROUND GALACTIC CEPHEIDS
Cepheid masses are a fundamental parameter for studying the pulsation and evolution of intermediate-mass stars, however the determination of their values is a long-standing problem since decades. Most of Cepheid masses are derived using stellar evolution or pulsation models, but they differ by 1 0-2...
Gorde:
| Argitaratua izan da: | Revista Mexicana de Astronomía y Astrofísica |
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| Egile nagusia: | |
| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
Universidad Nacional Autónoma de México
2015
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| Gaiak: | |
| Sarrera elektronikoa: | https://www.redalyc.org/articulo.oa?id=57150514008 |
| Etiketak: |
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