The stellar halo in Local Group Hestia simulations III. Chemical abundance relations for accreted and in situ stars (2023)

First Author: Khoperskov S
Attributed to:  GalaHAD: Galaxy Formation With High Accuracy Dynamics funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/202244234

Publication URI: http://dx.doi.org/10.1051/0004-6361/202244234

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics