48 citations
- New Mexico State UniversityUS6 papers
- Universidad Nacional Autónoma de MéxicoMX5 papers
- Brera Astronomical ObservatoryIT1 paper
- Brown UniversityUS1 paper
- California State University, FullertonUS1 paper
- Duke UniversityUS1 paper
- Institute for Theoretical and Experimental PhysicsRU1 paper
- Joint Institute for Nuclear ResearchRU1 paper
- Lawrence Berkeley National LaboratoryUS1 paper
- Lawrence Livermore National LaboratoryUS1 paper
- Los Alamos National LaboratoryUS1 paper
- North Carolina State UniversityUS1 paper
6 papers · 1 filter
Properties of voids in the Local Volume
Anton Tikhonov, Anatoly Klypin
Current explanation of the overabundance of dark matter subhalos in the Local Group (LG) indicates that there maybe a limit on mass of a halo, which can host a galaxy. This idea ca…
Substructure and halo density profiles in a Warm Dark Matter scenario
P. Colin, V. Avila-Reese, O. Valenzuela
High-resolution cosmological N-body simulations were performed in order to study the substructure of Milky Way-like galactic halos and the density profiles of halos in a warm dark…
Formation and evolution of disk galaxies within cold dark matter halos
V. Avila-Reese, C. Firmani, A. Klypin +1
We present results of extensive model calculations of disk galaxy evolution within an hierarchical inside-out formation scenario. We first compare properties of the dark halos iden…
Disk galaxy formation and evolution: models up to intermediate redshifts
C. Firmani, V. Avila-Reese
Making use of a seminumerical method we develop a scenario of disk galaxy formation and evolution in the framework of inflationary cold dark matter (CDM) cosmologies. Within the vi…
Dark Halos and Galaxy Evolution
C. Firmani, V. Avila-Reese
We study the evolution of disk galaxies within the frame of the cold dark matter (CDM) cosmologies. The hydrodynamics of a centrifugally supported gaseous disk and the growth of a…
On the Formation of Bulges and Elliptical Galaxies in the Cosmological Context
V. Avila-Reese, C. Firmani
We study the formation of hot spheroidal systems within the frame of a scenario where galaxy formation and evolution is related to the gentle mass aggregation history and primordia…