BINARY NATURE OF THE HADS STARS AN LYN & BE LYN

From newly determined times of maxima from CCD photometry of the HADS stars AN Lyn & BE Lyn and a compilation of previous times of maxima, we are able to determine the binary nature of these stars. We determine their physical parameters by means of uvby — β photometry.

Detalhes bibliográficos
Autores: J. H. Peña, A. Rentería, C. Villarreal, A. Pani, H. Huepa, J. L. Huepa, A. Bernal, A. Arenas, C. García, R. León, O. Trejo, E. Colorado, M. Sánchez-Cruces, J. S. Rechy-García
Formato: artículo
Estado:Versión publicada
Fecha de publicación:2015
País:México
Recursos:Universidad Nacional Autónoma de México
Repositorio:Redalyc-UNAM
OAI Identifier:oai:redalyc.org:57142745006
Acesso em linha:https://www.redalyc.org/articulo.oa?id=57142745006
Access Level:acceso abierto
Palavra-chave:Física, Astronomía y Matemáticas
stars
Binaries
variables
delta Scuti
Descrição
Resumo:From newly determined times of maxima from CCD photometry of the HADS stars AN Lyn & BE Lyn and a compilation of previous times of maxima, we are able to determine the binary nature of these stars. We determine their physical parameters by means of uvby — β photometry.

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