A study of the long term behavior of the SX PHE star KZ HYA1
From the newly determined times of maximum light of the SX Phe star KZ Hya and others from the literature, as well as from uvby − β photoelectric photometry, we determined the nature of this star and its physical parameters.
Збережено в:
| Опубліковано в:: | Revista Mexicana de Astronomía y Astrofísica |
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| Автори: | , , , , , , |
| Формат: | Artigo |
| Мова: | Inglês |
| Опубліковано: |
Universidad Nacional Autónoma de México
2018
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| Предмети: | |
| Онлайн доступ: | https://www.redalyc.org/articulo.oa?id=57171626006 https://www.redalyc.org/journal/571/57171626006/ https://www.redalyc.org/journal/571/57171626006/html/ https://www.redalyc.org/journal/571/57171626006/57171626006.epub https://www.redalyc.org/journal/571/57171626006/movil |
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