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

YEŞİLYAPRAK, Cahit; YERLİ, SİNAN; Gucsav, B.; Aksaker, NAZIM; Dikicioglu, E.; Helvaci, M.; Coker, D.; Aydin, M.; Dincel, B.; Uzun, N.

doi:10.1016/j.newast.2011.11.010

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

Atıf İçin Kopyala

YEŞİLYAPRAK C., YERLİ S. K., Gucsav B. B., Aksaker N., Dikicioglu E., Helvaci M., ...Daha Fazla

NEW ASTRONOMY, cilt.17, sa.5, ss.504-513, 2012 (SCI-Expanded)

Yayın Türü: Makale / Tam Makale
Cilt numarası: 17 Sayı: 5
Basım Tarihi: 2012
Doi Numarası: 10.1016/j.newast.2011.11.010
Dergi Adı: NEW ASTRONOMY
Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
Sayfa Sayıları: ss.504-513
Çukurova Üniversitesi Adresli: Evet

Özet

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 (C) 2011 Published by Elsevier B.V. All rights reserved.