Multi-component, axisymmetric dynamical models of dSphs based on distribution functions: inferences on dark matter and intermediate-mass black holes in Draco and Ursa Minor

Fuente: arXiv

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Bibliographic Details
Main Authors:	Pascale, R., Battaglia, G., Arroyo-Polonio, J. M., Vasiliev, E., Nipoti, C., Thomas, G. F.
Format:	Preprint
Published:	2026
Subjects:	Astrophysics of Galaxies
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2604.24855