Autor:
Caffau, E.
Gallagher, A.J.
Bonifacio, P.
Spite, M.
Duffau, S.
Spite, F.
Monaco, L.
Sbordone, L.
Aims. Carbon-enhanced metal-poor (CEMP) stars represent a sizeable fraction of all known metal-poor stars in the Galaxy. Their formation and composition remains a significant topic of investigation within the stellar astrophysics community. Methods. We analysed a sample of low-resolution spectra ...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/9238
Caffau, E.
,
Gallagher, A.J.
,
Bonifacio, P.
,
Spite, M.
,
Duffau, S.
,
Spite, F.
,
Monaco, L.
,
Sbordone, L.
,
[Investigation of a sample of carbon-enhanced metal-poor stars observed with FORS and GMOS]
,
Investigation of a sample of carbon-enhanced metal-poor stars observed with FORS and GMOS
