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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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. |
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Format: | Digital revista |
Language: | English |
Published: |
Universidad Nacional Autónoma de México, Instituto de Astronomía
2015
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Online Access: | http://www.scielo.org.mx/scielo.php?script=sci_arttext&pid=S0185-11012015000100006 |
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