On the origin of the kinematical differences between the stellar halo and the old globular cluster system in the Large Magellanic Cloud
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/380/4/1669/18689618/mnras0380-1669.pdf
Reference58 articles.
1. The Stellar Halo in the Large Magellanic Cloud: Mass, Luminosity, and Microlensing Predictions
2. The Globular Cluster System of the Virgo Dwarf Elliptical Galaxy VCC 1087
3. The Galactic Globular Cluster System as a Fossil Record of Reionization
4. Formation of the Galactic Stellar Halo: Origin of the Metallicity-Eccentricity Relation
5. Formation of the Galactic Stellar Halo. I. Structure and Kinematics
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1. Two kinematically distinct old globular cluster populations in the Large Magellanic Cloud;Monthly Notices of the Royal Astronomical Society: Letters;2018-12-28
2. THE AGE-METALLICITY RELATIONSHIP OF THE LARGE MAGELLANIC CLOUD FIELD STAR POPULATION FROM WIDE-FIELD WASHINGTON PHOTOMETRY;The Astronomical Journal;2012-12-12
3. Unearthing foundations of a cosmic cathedral: searching the stars for M33's halo;Monthly Notices of the Royal Astronomical Society;2012-10-29
4. Origin of Structural and Kinematic Properties of the Small Magellanic Cloud;Publications of the Astronomical Society of Australia;2009
5. Models for the dynamical evolution of the Magellanic System;Proceedings of the International Astronomical Union;2008-07
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