A study of the long term behavior of the SX PHE star KZ HYA
Abstract 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 − β photoelectric photometry, we determined the nature of this star and its physical parameters.
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| Main Authors: | , , , , , , |
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| Format: | Digital revista |
| Language: | English |
| Published: |
Universidad Nacional Autónoma de México, Instituto de Astronomía
2018
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| Online Access: | http://www.scielo.org.mx/scielo.php?script=sci_arttext&pid=S0185-11012018000100006 |
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