A STUDY OF THE LONG TERM BEHAVIOR OF THE SX PHE STAR KZ HYA
Por:
Pena, J. H., Pina, D. S., Renteria, A., Villarreal, C., Soni, A. A., Guillen, J., Calderon, J.
Publicada:
1 abr 2018
Resumen:
From the newly determined times of maximum light of the SX Phe star KZ
Hya and others from the literature, as well as from uvby - beta
photoelectric photometry, we determined the nature of this star and its
physical parameters.
Filiaciones:
Pena, J. H.:
Univ Nacl Autonoma Mexico, Inst Astron, Apdo Postal 70-264, Mexico City, DF, Mexico
Observ Astron Nacl, Tonantzintla, Mexico
Univ Nacl Autonoma Mexico, Fac Ciencias, Mexico City, DF, Mexico
Pina, D. S.:
Univ Nacl Autonoma Mexico, Inst Astron, Apdo Postal 70-264, Mexico City, DF, Mexico
Univ Nacl Autonoma Mexico, Fac Ciencias, Mexico City, DF, Mexico
Renteria, A.:
Univ Nacl Autonoma Mexico, Inst Astron, Apdo Postal 70-264, Mexico City, DF, Mexico
Univ Nacl Autonoma Mexico, Fac Ciencias, Mexico City, DF, Mexico
Villarreal, C.:
Univ Nacl Autonoma Mexico, Inst Astron, Apdo Postal 70-264, Mexico City, DF, Mexico
Univ Nacl Autonoma Mexico, Fac Ciencias, Mexico City, DF, Mexico
Soni, A. A.:
Univ Nacl Autonoma Mexico, Inst Astron, Apdo Postal 70-264, Mexico City, DF, Mexico
Univ Nacl Autonoma Mexico, Fac Ciencias, Mexico City, DF, Mexico
Guillen, J.:
Univ Nacl Autonoma Mexico, Inst Astron, Apdo Postal 70-264, Mexico City, DF, Mexico
Univ Nacl Autonoma Mexico, Fac Ciencias, Mexico City, DF, Mexico
Calderon, J.:
Univ Nacl Autonoma Mexico, Inst Astron, Apdo Postal 70-264, Mexico City, DF, Mexico
Univ Nacl Autonoma Mexico, Fac Ciencias, Mexico City, DF, Mexico
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