Context. Low-mass dwarf spheroidal galaxies are key objects for our understanding of the chemical evolution of the pristine Universe and the Local Group of galaxies. Abundance ratios in stars of these objects can be used to better understand their star formation and chemical evolution. Aims. We r...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/3983
François, P.
,
Monaco, L.
,
Bonifacio, P.
,
Moni Bidin, C.
,
Geisler, D.
,
[Abundance ratios of red giants in low-mass ultra-faint dwarf spheroidal galaxies]
,
Abundance ratios of red giants in low-mass ultra-faint dwarf spheroidal galaxies
