Explaining the chemical trajectories of accreted and in-situ halo stars of the Milky Way (2020)

First Author: Brook C
Attributed to:  MSSL/UCL Astrophysics Consolidated Grant 2016-2019 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2001.02187

Publication URI: https://arxiv.org/abs/2001.02187

Type: Other