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A study of the secular variation of the high-amplitude Delta Scuti star AD CMi

We determine the nature of the Delta Scuti star AD CMi and its physical parameters from newly determined times of maximum light and other times from the literature, as well as from uvby − β photoelectric photometry.

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Bibliografiske detaljer
Udgivet i:Revista Mexicana de Astronomía y Astrofísica
Principais autores: J. H. Peña, D. S. Piña, H. Huepa, S. B. Juárez, C. Villarreal, J. Guillén, A. A. Soni, A. Rentería, J. M. Donaire, R. R. Muñoz, T. Benadalid, J. D. Paredes, E. D. Orozco, I. Soberanes, H. Posadas, C. Castro, J. Briones, M. Romero, F. Martinez, A. L. Zuñiga, J. L. Carrillo, B. Chávez, D. Navez, C. García
Format: Artigo
Sprog:Inglês
Udgivet: Universidad Nacional Autónoma de México 2021
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Online adgang:https://www.redalyc.org/articulo.oa?id=57171643006
https://www.redalyc.org/journal/571/57171643006/
https://www.redalyc.org/journal/571/57171643006/html/
https://www.redalyc.org/journal/571/57171643006/57171643006.epub
https://www.redalyc.org/journal/571/57171643006/movil
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