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.
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| Опубликовано в:: | Revista Mexicana de Astronomía y Astrofísica |
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| Главные авторы: | , , , , , , |
| Формат: | Artigo |
| Язык: | Inglês |
| Опубликовано: |
Universidad Nacional Autónoma de México
2018
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| Предметы: | |
| Online-ссылка: | 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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