Bildiri
Tam Metin Bildiri
Uluslararası
2016
Colour relations for Mira and Semiregular (SR) type stars
1st International Physics Conference at the Anatolian Peak, IPCAP 2016
Erzurum · 25.02.2016–27.02.2016 · 25.02.2016
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.
Atıf için künye
Güney, Y., & Yeşilyaprak, C. (2016). Colour relations for Mira and Semiregular (SR) type stars. 1st International Physics Conference at the Anatolian Peak, IPCAP 2016, Erzurum. https://doi.org/10.1088/1742-6596/707/1/012044
BibTeX
@inproceedings{guney2016-57529,
author = {Güney, Yavuz and Yeşilyaprak, Cahit},
title = {Colour relations for Mira and Semiregular (SR) type stars},
booktitle = {1st International Physics Conference at the Anatolian Peak, IPCAP 2016},
address = {Erzurum},
year = {2016},
doi = {10.1088/1742-6596/707/1/012044},
url = {https://akademik.atauni.edu.tr/yayinlar/57529-colour-relations-for-mira-and-semiregular-sr-type-stars}
}