| Issue |
A&A
Volume 606, October 2017
|
|
|---|---|---|
| Article Number | C1 | |
| Number of page(s) | 1 | |
| Section | Galactic structure, stellar clusters and populations | |
| DOI | https://doi.org/10.1051/0004-6361/201630102e | |
| Published online | 27 October 2017 | |
Near-IR period-luminosity relations for pulsating stars in ω Centauri (NGC 5139) (Corrigendum)
1 Instituto de Astrofísica, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, 782-0436 Macul, Santiago, Chile
e-mail: cnavarre@astro.puc.cl; mcatelan@astro.puc.cl; rcontre@astro.puc.cl
2 Instituto Milenio de Astrofísica, Santiago, Chile
3 Centro de Astro-Ingeniería, Pontificia Universidad Católica de Chile, Santiago, Chile
4 Unidad de Astronomía, Facultad Cs. Básicas, Universidad de Antofagasta, Av. U. de Antofagasta 02800, Antofagasta, Chile
5 Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstr. 12-14, 69120 Heidelberg, Germany
6 Departamento de Fisica, Facultad de Ciencias Exactas, Universidad Andres Bello, Av. Fernandez Concha 700, Las Condes, Santiago, Chile
7 Vatican Observatory, V 00120 Vatican City State, Italy
This article has no abstract.
Key words: stars: variables: RR Lyrae / stars: variables: Cepheids / stars: variables: delta Scuti / globular clusters: individual: NGC 5139 / infrared: stars / errata, addenda
© ESO, 2017
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