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

YEŞİLYAPRAK C., YERLİ S. K., Güsav B., Aksaker N., Dikiciolu E., Helvaci M., ...Daha Fazla

New Astronomy, cilt.17, sa.5, ss.504-513, 2012 (SCI-Expanded) identifier

  • 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
  • Anahtar Kelimeler: Methods: data analysis, Stars: late-type
  • Ankara 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 TÜBTAK 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. © 2012 Elsevier B.V. All rights reserved.