collaborators

8 papers

astro-ph.GA2026

Structural Diversity Among the Milky Way's Dwarf Spheroidal Satellites

Matthew G. Walker, Raphaël Errani, Andrew B. Pace +3

We fit a flexible double power-law (`') model to the stellar density fields observed for the Milky Way's known dwarf spheroidal satellite galaxies. We show that where stand…

astro-ph.GA2026

Collisional Dynamics of Stars and Dark Matter in Ultra-Faint Galaxies

Raphaël Errani, Raphaël Errani, Nicolas Esser +3

We use controlled N-body simulations to study the collisional exchange of energy between stars and dark matter in ultra-faint galaxies. We find that dynamical friction between star…

astro-ph.GA2026

Stellar Cores Live Long and Prosper in Cuspy Dark Matter Halos

Jenni Häkkinen, Alexander Rawlings, Till Sawala +1

The existence of cuspy or cored centers of dark matter halos is a crucial discriminant between different dark matter models. It has recently been claimed based on dynamical argumen…

astro-ph.GA2026

Tailored mass estimators for Milky Way dwarf Spheroidals

Sofia L. Splawska, Raphaël Errani, Jorge Peñarrubia +1

Assuming spherical symmetry and dynamical equilibrium within a given gravitational potential, a dwarf spheroidal (dSph) galaxy's globally averaged stellar velocity dispersion depen…

astro-ph.GA2026

Signatures of dark subhalos in dwarf spheroidal galaxies: I. Fluctuations in surface density

Eduardo Vitral, Jorge Peñarrubia, Matthew G. Walker

Dark matter (DM) subhalos offer critical tests of cosmological models through their abundance and properties, yet most remain undetectable due to their lack of stars. We investigat…

astro-ph.GA2025

Stellar Mass Segregation in Dark Matter Halos

Raphaël Errani, Jorge Peñarrubia, Matthew G. Walker

We study the effect of stellar mass segregation driven by collisional relaxation within the potential well of a smooth dark matter halo. This effect is of particular relevance for…