The Formation and Evolution of Young Low-mass Stars within Halos with High Concentration of Dark Matter Particles

Abstract

The formation and evolution of low-mass stars within dense halos of dark matter (DM) leads to evolution scenarios quite different from the classical stellar evolution. As a result of our detailed numerical work, we describe these new scenarios for a range of DM densities on the host halo, a range of scattering cross sections of the DM particles considered… (More)

11 Figures and Tables

Topics

  • Presentations referencing similar topics