Autor:
Barbuy, B.
Muniz, L.
Ortolani, S.
Ernandes, H.
Dias, B.
Saviane, I.
Kerber, L.
Bica, E.
Pérez-Villegas, A.
Rossi, L.
Held, E.V.
Context. NGC 6558 is a bulge globular cluster with a blue horizontal branch (BHB), combined with a metallicity of [Fe/H] â‰-1.0. It is similar to HP 1 and NGC 6522, which could be among the oldest objects in the Galaxy. Element abundances in these clusters could reveal the nature of the first sup...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/11578
Barbuy, B.
,
Muniz, L.
,
Ortolani, S.
,
Ernandes, H.
,
Dias, B.
,
Saviane, I.
,
Kerber, L.
,
Bica, E.
,
Pérez-Villegas, A.
,
Rossi, L.
,
Held, E.V.
,
[High-resolution abundance analysis of four red giants in the globular cluster NGC 6558]
,
High-resolution abundance analysis of four red giants in the globular cluster NGC 6558
