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.

Authors: 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
Format: Article
Status:Published version
Publication date:2015
Country:México
Institution:UNAM
Repository:Redalyc-UNAM
OAI Identifier:oai:redalyc.org:57142745006
Online Access:https://www.redalyc.org/articulo.oa?id=57142745006
Access Level:Open access
Keyword:Física, Astronomía y Matemáticas
stars
Binaries
variables
delta Scuti
Summary: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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