Results of Observations of Maxima of Pulsating Stars

The systematic study of some HADS stars, recognized as variables for decades, has allowed us to provide data on their secular variations through O-C analysis. However, some of the data have large gaps without observations. This is our motivation for continuously observing these stars as part of the...

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Εκδόθηκε σε:	Revista Mexicana de Astronomía y Astrofísica
Κύριοι συγγραφείς:	J. H. Peña, H. Huepa, D. S. Piña, J. Guillén, A. Rentería, J. D. Paredes, R. Muñoz, J. Donaire, T. Benadalid
Μορφή:	Artigo
Γλώσσα:	Inglês
Έκδοση:	Universidad Nacional Autónoma de México 2021
Θέματα:	Física, Astronomía y Matemáticas
Διαθέσιμο Online:	https://www.redalyc.org/articulo.oa?id=57171634018 https://www.redalyc.org/journal/571/57171634018/ https://www.redalyc.org/journal/571/57171634018/html/ https://www.redalyc.org/journal/571/57171634018/57171634018.epub https://www.redalyc.org/journal/571/57171634018/movil
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