Julio F. Navarro

TL;DR: In this paper , the authors use N-body simulations to study the evolution of NFW-like "cored" subhaloes in the tidal field of a massive host, and identify the criteria and timescales for full disruption.

TL;DR: In this article, the authors compare the spherically-averaged circular velocity (V c ) profiles to the rotation curves of low surface brightness (LSB) galaxies in the samples of de Blok et al. and Swaters et al., showing that the V c profiles of simulated CDM halos are generally consistent with the rotation curve of LSB galaxies, but there are also some clearly discrepant cases.

TL;DR: In this paper, the rotation curve of the Milky Way in the extended solar neighbourhood using a sample of SEGUE (Sloan Extension for Galactic Understanding and Exploration) G-dwarfs was constructed.

TL;DR: This work confirms and extends earlier indications that the mass profiles of CDM haloes are roughly independent of mass and that the dark-matter density appears to diverge in a central ‘cusp’, and shows that CDM halo-density profiles get increasingly shallow inwards down to the innermost radius.

TL;DR: The C-19 stream is the most metal poor stellar system ever discovered, with a mean metallicity [Fe/H] = −3.38 ± 0.06 as discussed by the authors .