Long-term variations and periods of Mira stars from ROTSE–IIId

2012-7
Yeşilyaprak, C.
Yerli, Sinan Kaan
Güçsav, B.B.
Aksaker, N.
Dikicioğlu, E.
Helvacı, M.
Çoker, D.
Aydın, M.E.
Dinçel, B.
Uzun, N.
We have studied the long-term variations of Mira type variables observed with Robotic Optical Transient Search Experiment telescope (ROTSE-IIId) between 2004 and 2009 located at TUBITAK National Observatory (TUG) in Antalya, Turkey. The actual pulsation periods, variability amplitudes, epochs of maximums and light curves of selected 70 Mira type variables already defined in the SIMBAD database were investigated. In these variables; 17 periods are identified for the first time. Crown Copyright.

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Citation Formats
C. Yeşilyaprak et al., “Long-term variations and periods of Mira stars from ROTSE–IIId,” New Astronomy, pp. 504–513, 2012, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/28284.