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The edge of the Galaxy

Deason, AJ, Fattahi, A, Frenk, CS, Grand, RJJ, Oman, KA, Garrison-Kimmel, S, Simpson, CM and Navarro, JF (2020) The edge of the Galaxy. Monthly Notices of the Royal Astronomical Society, 496 (3). pp. 3929-3942. ISSN 0035-8711

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We use cosmological simulations of isolated MilkyWay (MW)-mass galaxies, as well as Local Group (LG) analogues, to define the 'edge'- A caustic manifested in a drop in density or radial velocity-of Galactic-sized haloes, both in dark matter and in stars. In the dark matter, we typically identify two caustics: The outermost caustic located at ∼1.4r200m, corresponding to the 'splashback' radius, and a second caustic located at ∼0.6r200m, which likely corresponds to the edge of the virialized material that has completed at least two pericentric passages. The splashback radius is ill defined in LG-type environments where the haloes of the two galaxies overlap. However, the second caustic is less affected by the presence of a companion, and is a more useful definition for the boundary of the MWhalo. Curiously, the stellar distribution also has a clearly defined caustic, which, in most cases, coincides with the second caustic of the darkmatter. This can be identified in both radial density and radial velocity profiles, and should be measurable in future observational programmes. Finally, we show that the second caustic can also be identified in the phase-space distribution of dwarf galaxies in the LG. Using the current dwarf galaxy population, we predict the edge of the MW halo to be 292 ± 61 kpc.

Item Type: Article
Uncontrolled Keywords: 0201 Astronomical and Space Sciences; Astronomy & Astrophysics
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Astrophysics Research Institute
Publisher: Oxford University Press (OUP)
SWORD Depositor: A Symplectic
Date Deposited: 18 Apr 2023 09:11
Last Modified: 18 Apr 2023 09:15
DOI or ID number: 10.1093/MNRAS/STAA1711
URI: https://researchonline.ljmu.ac.uk/id/eprint/19309
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