Colour relations for Mira and Semiregular (SR) type stars

GÜNEY Y., YEŞİLYAPRAK C.

1st International Physics Conference at the Anatolian Peak, IPCAP 2016, Erzurum, Türkiye, 25 - 27 Şubat 2016, cilt.707 identifier identifier

  • Yayın Türü: Bildiri / Tam Metin Bildiri
  • Cilt numarası: 707
  • Doi Numarası: 10.1088/1742-6596/707/1/012044
  • Basıldığı Şehir: Erzurum
  • Basıldığı Ülke: Türkiye
  • Atatürk Üniversitesi Adresli: Evet

Özet

In this study, the period-colour relations, the colour-colour relations and the effective temperature were examined for Semiregular (SR) and Mira type variable stars. SR variables show an obvious period-colour relations, especially in infrared (IR). There are differences between SR and Mira type variable stars with respect to their colour relations. It has been thought that these differencies are caused by their mass loss rates and their effective temperatures.