activity
19982026
most citedDipole formation at metal/PTCDA interfaces: Role of the Charge Neutrality Level

220 citations · 887 across the 30 of their papers we have counts for

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7 papers · 1 filter

astro-ph2008

Circumnuclear Regions of Star Formation in Early Type Galaxies

Angeles I. Diaz, Elena Terlevich, Guillermo F. Hagele +1

Circumnuclear star forming regions, also called hotspots, are often found in the inner regions of some spiral galaxies where intense processes of star formation are taking place. I…

astro-ph2007

The role of the star formation on the nitrogen abundance evolution

M. Mollá, J. M. Vílchez, A. I. Díaz +1

We analyze the evolution of nitrogen resulting from a set of spiral and irregular galaxy models computed for a large number of input mass radial distributions and with various star…

astro-ph2006★ 31 cited

A Spectroscopic Study of the Near-IR [SIII] Lines in a Sample of HII Galaxies: chemical abundances

C. Kehrig, J. M. Vilchez, E. Telles +2

A detailed spectroscopic study, from lambda 3700 A to 1 um, was performed for a sample of 34 HII galaxies in order to derive fundamental parameters for their HII regions and ionizi…

astro-ph2004★ 25 cited

Structural parameters of nearby emission-line galaxies

Miguel Sanchez-Portal, Angeles I Diaz, Elena Terlevich +1

We present the results of an investigation on the main structural properties derived from VRI and Halpha surface photometry of galaxies hosting nuclear emission-line regions (inclu…

astro-ph2003★ 152 cited

On the physical origin of dark matter density profiles

Y. Ascasibar, G. Yepes, S. Gottloeber +1

The radial mass distribution of dark matter haloes is investigated within the framework of the spherical infall model. We present a new formulation of spherical collapse including…

astro-ph2003★ 77 cited

The radial structure of galaxy groups and clusters

Y. Ascasibar, G. Yepes, V. Mueller +1

Simple self-consistent models of galaxy groups and clusters are tested against the results of high-resolution adiabatic gasdynamical simulations. We investigate two models based on…