Quantifying the smoothness of the stellar halo: a link to accretion history-Reference-Cited by-同舟云学术

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Quantifying the smoothness of the stellar halo: a link to accretion history

Published:2019-01-16 Issue:2 Volume:484 Page:2556-2565
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Lancaster Lachlan¹²^ORCID,Belokurov Vasily²³^ORCID,Evans N Wyn²

Affiliation:

1. Department of Astrophysical Sciences, Princeton University, 4 Ivy Lane, Princeton, NJ 08544, USA

2. Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK

3. Center for Computational Astrophysics, Flatiron Institute, 162 5th Avenue, New York, NY 10010, USA

Funder

European Research Council

European Union’s Seventh Framework Programme

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/484/2/2556/27643986/stz124.pdf

Reference89 articles.

1. Stars beyond galaxies: the origin of extended luminous haloes around galaxies

2. The Accretion Origin of the Milky Way’s Stellar Halo

3. The Field of Streams: Sagittarius and Its Siblings

4. Precession of the Sagittarius stream

5. The Discovery of Tidal Tails around the Globular Cluster NGC 5466

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2. Mapping the milky way’s stellar halo with 2D data;Monthly Notices of the Royal Astronomical Society;2023-07-31

3. On the edge: the relation between stellar and dark matter haloes of Milky Way-mass galaxies;Monthly Notices of the Royal Astronomical Society;2023-02-06

4. Two-point Correlation Function Studies for the Milky Way: Discovery of Spatial Clustering from Disk Excitations and Substructure;The Astrophysical Journal;2023-01-01

5. Walter: A Tool for Predicting Resolved Stellar Population Observations with Applications to the Roman Space Telescope;The Astronomical Journal;2022-09-16

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