文章基本信息

标题：Near-IR period-luminosity relations for pulsating stars in ω Centauri (NGC 5139) (Corrigendum)
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作者：C. Navarrete ; M. Catelan ; R. Contreras Ramos 等
期刊名称：Astronomy & Astrophysics
印刷版ISSN：0004-6361
电子版ISSN：1432-0746
出版年度：2017
卷号：606
页码：1-1
DOI：10.1051/0004-6361/201630102e
语种：English
出版社：EDP Sciences
摘要：An incorrect zero point for the empirical period-luminosity- metallicity (PL-Z) relations for RR Lyrae (RRL) stars in ω Cen- tauri (NGC5139) was inadvertently reported in Table 2 and Eqs. (4) and (5) of our original paper. The corrected table and equations are given below. The actual analysis that is described inthepaperwasbasedonthecorrectzeropoints,andsoallofthe results reported in our original publication remain unchanged.
关键词：enstars: variables: RR Lyraestars: variables: Cepheidsstars: variables: delta Scutiglobular clusters: individual: NGC 5139infrared: starserrata, addenda