271 citations · 716 across the 14 of their papers we have counts for
7 papers · 1 filter
How unique are pulsar wind nebulae models? Implementation of a multi-parameter, automatic fitting for time-dependent spectra
J. Martin, D. F. Torres
Due to the computational cost of calculating a great number of variations of the parameters, detailed radiative models of pulsar wind nebulae (PWNe) do not usually contain fitting…
Revisiting the evolution of nonradiative supernova remnants: A hydrodynamical-informed parameterization of the shock positions
R. Bandiera, N. Bucciantini, J. Martín +2
Understanding the evolution of a supernova remnant shell in time is fundamental. Such understanding is critical to build reliable models of the dynamics of the supernova remnant sh…
Reverberation of pulsar wind nebulae (I): Impact of the medium properties and other parameters upon the extent of the compression
R. Bandiera, N. Bucciantini, J. Martin +2
The standard approach to the long term evolution of pulsar wind nebulae (PWNe) is based on one-zone models treating the nebula as a uniform system. In particular for the late phase…
Exploring the effects of magnetar bursts in pulsar wind nebulae
J. Martin, D. F. Torres, B. Zhang
We explore possible effects of a magnetar burst on the radio, X-ray, and gamma-ray flux of a pulsar wind nebula (PWN). We assume that the burst injects electron-positron pairs or p…
Interacting supernovae and supernova impostors. LSQ13zm: an outburst heralds the death of a massive star
L. Tartaglia, A. Pastorello, M. Sullivan +37
We report photometric and spectroscopic observations of the optical transient LSQ13zm. Historical data reveal the presence of an eruptive episode (that we label as `2013a') followe…
Comparing supernova remnants around strongly magnetized and canonical pulsars
J. Martin, N. Rea, D. F. Torres +1
The origin of the strong magnetic fields measured in magnetars is one of the main uncertainties in the neutron star field. On the other hand, the recent discovery of a large number…