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

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Bibliographische Detailangaben
Hauptverfasser: Kovtyukh, Valery (VerfasserIn) , Lemasle, Bertrand (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 2018 March 14
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 477, Heft: 2, Pages: 2276-2285
ISSN:1365-2966
DOI:10.1093/mnras/sty671
Online-Zugang:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty671
Verlag, Volltext: https://academic.oup.com/mnras/article/477/2/2276/4935186
Volltext
Verfasserangaben:V. Kovtyukh, I. Yegorova, S. Andrievsky, S. Korotin, I. Saviane, B. Lemasle, F. Chekhonadskikh and S. Belik
Beschreibung
Zusammenfassung:Abstract. The chemical composition of 28 Population II Cepheids and one RR Lyrae variable has been studied using high-resolution spectra. The chemical composit
Beschreibung:Gesehen am 05.02.2019
Beschreibung:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/sty671