Type II Cepheids: evidence for Na-O anticorrelation for BL Her type stars?

Abstract. The chemical composition of 28 Population II Cepheids and one RR Lyrae variable has been studied using high-resolution spectra. The chemical composit

Saved in:
Bibliographic Details
Main Authors: Kovtyukh, Valery (Author) , Lemasle, Bertrand (Author)
Format: Article (Journal)
Language:English
Published: 2018 March 14
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 477, Issue: 2, Pages: 2276-2285
ISSN:1365-2966
DOI:10.1093/mnras/sty671
Online Access:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty671
Verlag, Volltext: https://academic.oup.com/mnras/article/477/2/2276/4935186
Get full text
Author Notes:V. Kovtyukh, I. Yegorova, S. Andrievsky, S. Korotin, I. Saviane, B. Lemasle, F. Chekhonadskikh and S. Belik
Description
Summary:Abstract. The chemical composition of 28 Population II Cepheids and one RR Lyrae variable has been studied using high-resolution spectra. The chemical composit
Item Description:Gesehen am 05.02.2019
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/sty671