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Near-IR period-luminosity relations for pulsating stars in [Omega] Centauri (NGC 5139)

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<i>Aims. <i/>The globular cluster <i>ω<i/> 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 rel...

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Main Authors: Navarrete, Camila (Author) , Dékány, István (Author)
Format: Article (Journal)
Language:English
Published: 24 August 2017
In: Astronomy and astrophysics
Year: 2017, Volume: 604, Pages: A120
ISSN:1432-0746
DOI:10.1051/0004-6361/201630102
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1051/0004-6361/201630102
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Author Notes:C. Navarrete, M. Catelan, R. Contreras Ramos, J. Alonso-García, F. Gran, I. Dékány, and D. Minniti
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Near-IR period-luminosity relations for pulsating stars in [Omega] Centauri (NGC 5139) by Navarrete, Camila (Author) , Dékány, István (Author) ,


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