Application of the Eddington inversion method to constrain the dark matter halo of galaxies using only observed surface brightness profiles
Context. The halos of low-mass galaxies may allow us to constrain the nature of dark matter (DM), but the kinematic measurements needed to diagnose the required properties are technically extremely challenging. However, the photometry of these systems is doable. Aims. Using only stellar photometry, we wanted to constrain key properties of the DM
Sánchez Almeida, Jorge et al.
Advertised on:
10
2024