The stellar halo in Local Group Hestia simulations. III. Chemical abundance relations for accreted and in situ stars
Stellar chemical abundances and kinematics provide key information for recovering the assembly history of galaxies. In this work we explore the chemo-chrono-kinematics of accreted and in situ stellar populations, by analyzing six M31/Milky Way (MW) analogues from the HESTIA suite of cosmological hydrodynamics zoom-in simulations of the Local Group
Khoperskov, Sergey et al.
Fecha de publicación:
9
2023