Characterisation of local halo building blocks: Thamnos and Sequoia
Context. A crucial aspect of galaxy evolution is the pace at which galaxies build up their mass. We can investigate this hierarchical assembly by uncovering and timing accretion events experienced by our Galaxy. Aims. In the Milky Way, accreted debris has been previously identified in the local halo, thanks to the advent of Gaia data. We aim to
Dodd, Emma et al.
Fecha de publicación:
6
2025