activity
19972007
most citedThe HI Content of Spirals. II. Gas Deficiency in Cluster Galaxies

365 citations · 467 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph2007★ 42 cited

The nature of dark matter and the density profile and central behavior of relaxed halos

Eduard Salvador-Solé, Alberto Manrique, Guillermo González-Casado +1

We show that the two basic assumptions of the model recently proposed by Manrique and coworkers for the universal density profile of cold dark matter (CDM) halos, namely that these…

astro-ph2005★ 13 cited

Implications of Halo Inside-out Growth on the X-Ray Properties of Nearby Galaxy Systems within the Preheating Scenario

Jose M. Solanes, Alberto Manrique, Guillermo Gonzalez-Casado +1

We present an entirely analytic model for a preheated, polytropic intergalactic medium in hydrostatic equilibrium within a NFW dark halo potential in which the evolution of the hal…

astro-ph2000★ 365 cited

The HI Content of Spirals. II. Gas Deficiency in Cluster Galaxies

Jose M. Solanes, Alberto Manrique, Carlos Garcia-Gomez +3

We derive the atomic hydrogen content for a total of 1900 spirals in the fields of eighteen nearby clusters. By comparing the HI deficiency distributions of the galaxies inside of…

astro-ph1998★ 2 cited

Substructure in the ENACS clusters

J. M. Solanes, E. Salvador-Sole, G. Gonzalez-Casado

Subclustering is investigated in a set of 67 rich cluster galaxy samples extracted from the ESO Nearby Abell Cluster Survey (ENACS) catalog. We apply four well-known statistical te…

astro-ph1998

Why are Halo Density Profiles Stable at Formation?

G. Gonzalez-Casado, A. Raig, E. Salvador-Sole

We analyze the physical justification of the picture proposed by Salvador-Sole et al. in these proceedings for the time evolution of the universal density profile of dark-matter ha…

astro-ph1998★ 20 cited

Scaling Evolution of Universal Dark-Matter Halo Density Profiles

A. Raig, G. Gonzalez-Casado, E. Salvador-Sole

Dark-matter halos show a universal density profile with a scaling such that less massive systems are typically denser. This mass-density relation is well described by a proportiona…