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19952018
most citedSubstructure and halo density profiles in a Warm Dark Matter Cosmology

414 citations · 2.1k across the 29 of their papers we have counts for

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Showing astro-ph.GAShow all

8 papers · 1 filter

astro-ph.GA2018★ 22 cited

The global and radial stellar mass assembly of Milky Way-sized galaxies

V. Avila-Reese, A. González-Samaniego, P. Colín +2

We study the global and radial stellar mass assembly of eight zoomed-in MW-sized galaxies produced in Hydrodynamics cosmological simulations. The disk-dominated galaxies (4) show a…

astro-ph.GA2016★ 130 cited

Hierarchical Cluster Assembly in Globally Collapsing Clouds

Enrique Vazquez-Semadeni, Alejandro Gonzalez-Samaniego, Pedro Colin

We discuss the mechanism of cluster formation in a numerical simulation of a molecular cloud (MC) undergoing global hierarchical collapse (GHC). The global nature of the collapse i…

astro-ph.GA2016★ 24 cited

Cosmological simulations of Milky Way-sized galaxies

Pedro Colin, Vladimir Avila-Reese, Santi Roca-Fabrega +1

We introduce a new set of eight Milky Way-sized cosmological simulations performed using the AMR code ART + Hydrodynamics in a LCDM cosmology. The set of zoom-in simulations covers…

astro-ph.GA2016

Cluster Assembly in Hierarchically Collapsing Clouds

Enrique Vazquez-Semadeni, Alejandro Gonzalez-Samaniego, Manuel Zamora-Aviles +1

We discuss the mechanism of cluster formation in hierarchically collapsing molecular clouds. Recent evidence, both observational and numerical, suggests that molecular clouds (MCs)…

astro-ph.GA2014★ 37 cited

Simulations of galaxies formed in warm dark matter halos of masses at the filtering scale

Pedro Colin, Vladimir Avila-Reese, Alejandro Gonzalez-Samaniego +1

We present zoom-in N-body + Hydrodynamic simulations of dwarf central galaxies formed in Warm Dark Matter (WDM) halos with masses at present-day of \msun. Two d…

astro-ph.GA2014★ 1 cited

Supermassive Black Hole Binaries: Environment and Galaxy Host Properties of PTA and eLISA sources

Eva Martínez Palafox, Octavio Valenzuela, Pedro Colín +1

Supermassive black hole (BH) binaries would comprise the strongest sources of gravitational waves (GW) once they reach <<1 pc separations, for both pulsar timing arrays (PTAs) and…