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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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Detalles Bibliográficos
Publicado en:Revista Mexicana de Astronomía y Astrofísica
Principais autores: J. H. Peña, D. S. Piña, A. Rentería, C. Villarreal, A. A. Soni, J. Guillen, J. Calderón
Formato: Artigo
Idioma:Inglês
Publicado: Universidad Nacional Autónoma de México 2018
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Acceso en liña:https://www.redalyc.org/articulo.oa?id=57171626006
https://www.redalyc.org/journal/571/57171626006/
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https://www.redalyc.org/journal/571/57171626006/57171626006.epub
https://www.redalyc.org/journal/571/57171626006/movil
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