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Morphology of stellar populations in the Magellanic Clouds using the VMC survey

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arxiv 1810.03365 v1 pith:DEB7ECZ5 submitted 2018-10-08 astro-ph.GA astro-ph.SR

Morphology of stellar populations in the Magellanic Clouds using the VMC survey

Dalal El Youssoufi , Maria-Rosa L. Cioni , Cameron P. M. Bell , Stefano Rubele , Florian Niederhofer , Gal Matijevic This is my paper
classification astro-ph.GA astro-ph.SR
keywords magellaniccloudsstellarcloudinteractioninteractionsmilkymorphology
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The Magellanic Clouds are nearby dwarf irregular galaxies that represent a unique laboratory for studying galaxy interactions. Their morphology and dynamics have been heavily influenced by their mutual interactions as well as with their interaction(s) with the Milky Way. We use the VISTA near-infrared YJKs survey of the Magellanic Clouds system (VMC) in combination with stellar partial models of the Large Magellanic Cloud (LMC), the Small Magellanic Cloud (SMC) and the Milky Way to investigate the spatial distribution of stellar populations of different ages across the Magellanic Clouds. In this contribution, we present the results of these studies that allow us to trace substructures possibly related to the interaction history of the Magellanic Clouds.

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  1. The VMC survey -- LV. The coherent expansion of the SMC

    astro-ph.GA 2026-06 unverdicted novelty 4.0

    Improved VMC proper motions show SMC expansion along SE-NW axes consistent with LMC tides, radial inward motions with no rotation, and northward motion in older RGB stars from a prior interaction.