Abstract
We have carried out CCD photometry of KZ Hya from June 2004 to April 2007. With the 45 cm reflecting telescope donated by Japanese Official Development Assistance, we obtained 20 light maxima at the Astronomical Observatory of the National University of Asuncion in Paraguay. In addition, we have partly obtained three light maxima at the Gunma Astronomical Observatory in Japan. We have collected additional maximum data from literatures and data bases. The O − C values of KZ Hya varies sinusoidally with a period of 7.96 years, which supports the binary nature of KZ Hya suggested by some other workers. We have also clearly detected the secondary maximum of 0.03 mag at the phase of 0.66 on the light curve. The secondary maximum is found to have been present at the same phase since 1975 when KZ Hya was discovered as a pulsating variable star.
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Doncel, F., Momiyama, T. (2010). Period Study and Secondary Maximum of KZ Hya. In: Haubold, H., Mathai, A. (eds) Proceedings of the Third UN/ESA/NASA Workshop on the International Heliophysical Year 2007 and Basic Space Science. Astrophysics and Space Science Proceedings. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-03325-4_15
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DOI: https://doi.org/10.1007/978-3-642-03325-4_15
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