Binary nature of the HADS stars AN Lyn & BE Lyn

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.

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Bibliographic Details
Main Authors: Peña,J. H., Rentería,A., Villarreal,C., Pani,A., Huepa,H., Huepa,J. L., Bernal,A., Arenas,A., García,C., León,R., Trejo,O., Colorado,E., Sánchez-Cruces,M., Rechy-García,J. S.
Format: Digital revista
Language:English
Published: Universidad Nacional Autónoma de México, Instituto de Astronomía 2015
Online Access:http://www.scielo.org.mx/scielo.php?script=sci_arttext&pid=S0185-11012015000100006
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http://www.scielo.org.mx/scielo.php?script=sci_arttext&pid=S0185-11012015000100006

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