Autor:
Fernández-Alvar, E.
Carigi, L.
Schuster, W.J.
Hayes, C.R.
Ávila-Vergara, N.
Majewski, S.R.
Allende Prieto, C.
Beers, T.C.
Sánchez, S.F.
Zamora, O.
García-Hernández, D.A.
Tang, B.
Fernández-Trincado, J.G.
Tissera, P.
Geisler, D.
Villanova, S.
The formation processes that led to the current Galactic stellar halo are still under debate. Previous studies have provided evidence for different stellar populations in terms of elemental abundances and kinematics, pointing to different chemical and star formation histories (SFHs). In the prese...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/6361
Fernández-Alvar, E.
,
Carigi, L.
,
Schuster, W.J.
,
Hayes, C.R.
,
Ávila-Vergara, N.
,
Majewski, S.R.
,
Allende Prieto, C.
,
Beers, T.C.
,
Sánchez, S.F.
,
Zamora, O.
,
García-Hernández, D.A.
,
Tang, B.
,
Fernández-Trincado, J.G.
,
Tissera, P.
,
Geisler, D.
,
Villanova, S.
,
[Disentangling the Galactic Halo with APOGEE. II. Chemical and Star Formation Histories for the Two Distinct Populations]
,
Disentangling the Galactic Halo with APOGEE. II. Chemical and Star Formation Histories for the Two Distinct Populations
