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Impulsive Mixing of Stellar Populations in Dwarf Spheroidal Galaxies

We study the response of mono-energetic stellar populations with initially isotropic kinematics to impulsive and adiabatic changes to an underlying dark matter potential. Half-light radii expand and velocity dispersions decrease as enclosed dark matter is removed. The details of this expansion and c...

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Bibliografiset tiedot
Päätekijät: Raphaël Errani, Matthew G. Walker, Simon Rozier, Jorge Peñarrubia, Julio F. Navarro
Aineistotyyppi: Artigo
Kieli:Inglês
Julkaistu: IOP Publishing 2025-01-01
Sarja:The Astrophysical Journal
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Linkit:https://doi.org/10.3847/1538-4357/adfa27
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