The Magellanic Edges Survey I: Description and first results
Date
2020
Authors
Cullinane, Lara
Mackey, Dougal
Da Costa, Gary
Koposov, Sergey
Belokurov, Vasily
Erkal, Denis
Koch, A
Kunder, A
Nataf, David M
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Volume Title
Publisher
Blackwell Publishing Ltd
Abstract
We present an overview of, and first science results from, the Magellanic Edges Survey (MagES), an ongoing spectroscopic survey mapping the kinematics of red clump and red giant branch stars in the highly substructured periphery of the Magellanic Clouds. In conjunction with Gaia astrometry, MagES yields a sample of ∼7000 stars with individual 3D velocities that probes larger galactocentric radii than most previous studies. We outline our target selection, observation strategy, data reduction, and analysis procedures, and present results for two fields in the northern outskirts (>10◦ on-sky from the centre) of the Large Magellanic Cloud (LMC). One field, located in the vicinity of an arm-like overdensity, displays apparent signatures of perturbation away from an equilibrium disc model. This includes a large radial velocity dispersion in the LMC disc plane, and an asymmetric line-of-sight velocity distribution indicative of motions vertically out of the disc plane for some stars. The second field reveals 3D kinematics consistent with an equilibrium disc, and yields Vcirc = 87.7 +- 8.0 km s-1 at a radial distance of ∼10.5 kpc from the LMC centre. This leads to an enclosed mass estimate for the LMC at this radius of (1.8 +- 0.3) x 1010 M.
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Keywords
stars: kinematics and dynamics, galaxies: kinematics and dynamics, Magellanic Clouds, galaxies: stellar content, galaxies: structure
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Source
Monthly Notices of the Royal Astronomical Society
Type
Journal article
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Open Access
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