Autor:
Kovtyukh, V.
Yegorova, I.
Andrievsky, S.
Korotin, S.
Saviane, I.
Lemasle, B.
Chekhonadskikh, F.
Belik, S.
The chemical composition of 28 Population II Cepheids and one RR Lyrae variable has been studied using high-resolution spectra. The chemical composition of W Vir variable stars (with periods longer than 8 d) is typical for the halo and thick disc stars. However, the chemical composition of BL Her...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/8924
Kovtyukh, V.
,
Yegorova, I.
,
Andrievsky, S.
,
Korotin, S.
,
Saviane, I.
,
Lemasle, B.
,
Chekhonadskikh, F.
,
Belik, S.
,
[Type II Cepheids: Evidence for Na-O anticorrelation for BL Her type stars?]
,
Type II Cepheids: Evidence for Na-O anticorrelation for BL Her type stars?
