activity
19972026
most citedUnifying the observational diversity of isolated neutron stars via magneto-thermal evolution models

443 citations · 9.8k across the 192 of their papers we have counts for

collaborators
Showing 2002Show all

8 papers · 1 filter

astro-ph2002★ 16 cited

Time-Dependent Photoionization in a Dusty Medium. III: The effect of dust on the photoionization of metals

Davide Lazzati, Rosalba Perna

We use the time-dependent photoionization and dust destruction code developed by Perna & Lazzati (2002) to study the time evolution of the medium in a dusty gaseous cloud illuminat…

astro-ph2002★ 111 cited

Time-Dependent Photoionization in a Dusty Medium II: Evolution of Dust Distributions and Optical Opacities

Rosalba Perna, Davide Lazzati, Fabrizio Fiore

The interaction of a radiation field with a dusty medium is a relevant issue in several astrophysical contexts. We use the time-dependent photoionization code in a dusty medium dev…

astro-ph2002★ 46 cited

Broadband Modeling of GRB 021004

Jeremy S. Heyl, Rosalba Perna

We present a broadband modeling of the afterglow of GRB 021004. The optical transient of this burst has been detected very early and densely sampled in several bands. Its light cur…

astro-ph2002★ 356 cited

Neutrino trapping and accretion models for Gamma-Ray Bursts

Tiziana Di Matteo, Rosalba Perna, Ramesh Narayan

Many models of Gamma Ray Bursts invoke a central engine consisting of a black hole of a few solar masses accreting matter from a disk at a rate of a fraction to a few solar masses…

astro-ph2002★ 98 cited

Time-Dependent Photoionization in a Dusty Medium I: Code Description and General Results

Rosalba Perna, Davide Lazzati

We present a time-dependent photoionization code that combines self-consistently metal evolution and dust destruction under an intense X-ray UV radiation field. Firstly, we extend…

astro-ph2002★ 17 cited

A Self-Similar Solution for the Propagation of a Relativistic Shock in an Exponential Atmosphere

Rosalba Perna, Mario Vietri

We derive a fully relativistic, self-similar solution to describe the propagation of a shock along an exponentially decreasing atmosphere, in the limit of very large Lorentz factor…