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astro-ph2005

The maximum contribution to reionization from metal-free stars

Jose M. Rozas, Jordi Miralda-Escude, Eduard Salvador-Sole

We estimate the maximum contribution to reionization from the first generation of massive stars, with zero metallicity, under the assumption that one of these stars forms with a fi…

astro-ph2005

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-ph2005

Scale Radii and Aggregation Histories of Dark Haloes

Eduard Salvador-Sole, Alberto Manrique, Jose M. Solanes

Relaxed dark-matter haloes are found to exhibit the same universal density profiles regardless of whether they form in hierarchical cosmologies or via spherical collapse. Likewise,…

astro-ph2004

The origin of HI-deficiency in galaxies on the outskirts of the Virgo cluster. II. Companions and uncertainties in distances and deficiencies

T. Sanchis, G. A. Mamon, E. Salvador-Sole' +2

The origin of the deficiency in neutral Hydrogen of 13 spiral galaxies lying in the outskirts of the Virgo cluster is reassessed. If these galaxies have passed through the core of…

astro-ph2003

On the Origin of the Inner Structure of Halos

Alberto Manrique, Andreu Raig, Eduard Salvador-Sole +2

We calculate by means of the Press-Schechter formalism the density profile developed by dark-matter halos during accretion, i.e., the continuous aggregation of small clumps. We fin…

astro-ph2002

Major Mergers of Haloes, Growth of Massive Black Holes and Evolving Luminosity Function of Quasars

Evanthia Hatziminaoglou, Guy Mathez, Jose-Maria Solanes +2

We construct a physically motivated analytical model for the quasar luminosity function, based on the joint star formation and feeding of massive black holes suggested by the obser…