Meenakshi, P; Goswami, A; Doddamani, V. H
(Societe Royale des Sciences de Liege, 2019-10)
The halo system of the Milky way comprises the vast majority of the presently observed metal-poor ([Fe/H] <1.0) and very metal-poor ([Fe/H] <2.0) stars. A sizable fraction (~ 30%) of the metal-poor stars with carbon ...