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Constraints on the Formation of M31’s Stellar Halo from the SPLASH Survey

1
Space Telescope Science Institute, 3700 San Martin Dr, Baltimore, MD 21218, USA
2
Department of Physics & Astronomy, Johns Hopkins University, Baltimore, MD 21218, USA
Academic Editors: Duncan A. Forbes and Ericson D. Lopez
Galaxies 2017, 5(4), 59; https://doi.org/10.3390/galaxies5040059
Received: 16 August 2017 / Revised: 12 September 2017 / Accepted: 13 September 2017 / Published: 30 September 2017
(This article belongs to the Special Issue On the Origin (and Evolution) of Baryonic Galaxy Halos)
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Abstract

The SPLASH (Spectroscopic and Photometric Landscape of Andromeda’s Stellar Halo) Survey has observed fields throughout M31’s stellar halo, dwarf satellites, and stellar disk. The observations and derived measurements have either been compared to predictions from simulations of stellar halo formation or modeled directly in order to derive inferences about the formation and evolution of M31’s stellar halo. We summarize some of the major results from the SPLASH survey and the resulting implications for our understanding of the build-up of M31’s stellar halo. View Full-Text
Keywords: galaxies: evolution; galaxies: halos; galaxies: individual (M31) galaxies: evolution; galaxies: halos; galaxies: individual (M31)
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This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited (CC BY 4.0).
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Gilbert, K. Constraints on the Formation of M31’s Stellar Halo from the SPLASH Survey. Galaxies 2017, 5, 59.

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