Near-IR period-luminosity relations for pulsating stars in [Omega] Centauri (NGC 5139)
$\omega$ Centauri (NGC 5139) hosts hundreds of pulsating variable stars of different types, thus representing a treasure trove for studies of their corresponding period-luminosity (PL) relations. Our goal in this study is to obtain the PL relations for RR Lyrae, and SX Phoenicis stars in the field o...
Saved in:
| Main Authors: | , |
|---|---|
| Format: | Article (Journal) Chapter/Article |
| Language: | English |
| Published: |
2017
|
| In: |
Arxiv
|
| Online Access: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1704.03031
|
| Author Notes: | C. Navarrete, M. Catelan, R. Contreras Ramos, J. Alonso-García, F. Gran, I. Dékány, and D. Minniti |
Search Result 1