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Paper: |
Andromeda and its Satellites: A Kinematic Perspective |
Volume: |
458, Galactic Archaeology: Near-Field Cosmology and the Formation of the Milky Way |
Page: |
319 |
Authors: |
Collins, M. L. M.; Rich, R. M.; Chapman, S. C. |
Abstract: |
Using spectroscopic data taken with Keck II DEIMOS by the Z-PAndAS team in
the Andromeda-Triangulum region, I present a comparison of the disc and
satellite systems of Andromeda with those of our own Galaxy. I discuss the
observed discrepancies between the masses and scale radii of Andromeda dwarf
spheroidal galaxies of a given luminosity with those of the Milky Way. I
also present an analysis of the newly discovered M31 thick disc, which
is measured to be hotter, more extended and thicker than that seen in the
Milky Way. |
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