Autor:
Barbuy, B.
Cantelli, E.
Vemado, A.
Ernandes, H.
Ortolani, S.
Saviane, I.
Bica, E.
Minniti, D.
Dias, B.
Momany, Y.
Hill, V.
Zoccali, M.
Siqueira-Mello, C.
Context. The globular cluster HP 1 is projected at only 3.̊33 from the Galactic center. Together with its distance, this makes it one of the most central globular clusters in the Milky Way. It has a blue horizontal branch (BHB) and a metallicity of [Fe/H] ≈ −1.0. This means that it probably is on...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/2787
Barbuy, B.
,
Cantelli, E.
,
Vemado, A.
,
Ernandes, H.
,
Ortolani, S.
,
Saviane, I.
,
Bica, E.
,
Minniti, D.
,
Dias, B.
,
Momany, Y.
,
Hill, V.
,
Zoccali, M.
,
Siqueira-Mello, C.
,
[High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP 1]
,
High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP 1
