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

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

Jul 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012newa...17..504y&link_type=abstract

New Astronomy, Volume 17, Issue 5, p. 504-513.

Astronomy and Astrophysics

Astronomy

Scientific paper

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 TÜBİTAK 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.

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