Autor:
Sbordone, L.
Monaco, L.
Moni Bidin, C.
Bonifacio, P.
Villanova, S.
Bellazzini, M.
Ibata, R.
Chiba, M.
Geisler, D.
Caffau, E.
Duffau, S.
Context. The tidal disruption of the Sagittarius dwarf spheroidal galaxy (Sgr dSph) is producing the most prominent substructure in the Milky Way (MW) halo, the Sagittarius Stream. Aside from field stars, it is suspected that the Sgr dSph has lost a number of globular clusters (GC). Many Galactic...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/3763
Sbordone, L.
,
Monaco, L.
,
Moni Bidin, C.
,
Bonifacio, P.
,
Villanova, S.
,
Bellazzini, M.
,
Ibata, R.
,
Chiba, M.
,
Geisler, D.
,
Caffau, E.
,
Duffau, S.
,
[Chemical abundances of giant stars in NGC 5053 and NGC 5634, two globular clusters associated with the Sagittarius dwarf spheroidal galaxy?]
,
Chemical abundances of giant stars in NGC 5053 and NGC 5634, two globular clusters associated with the Sagittarius dwarf spheroidal galaxy?
