activity
20202026
most citedReverberation of pulsar wind nebulae (I): Impact of the medium properties and other parameters upon the extent of the compression

29 citations · 34 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2026★ 2 cited

Population synthesis of Galactic middle-aged pulsar wind nebulae I. Detection prospects for current and future instruments

A. De Sarkar, D. F. Torres, B. Olmi +2

Pulsar wind nebulae (PWNe) constitute the largest population of Galactic very-high-energy (VHE; GeV) -ray sources and are key laboratories for studying particle accele…

astro-ph.HE2026

Population synthesis of Galactic middle-aged pulsar wind nebulae II. Observational signatures of superefficiency

D. F. Torres, A. De Sarkar, B. Olmi +2

Pulsar wind nebulae (PWNe) interacting with the host supernova remnants (SNRs) can enter the reverberation phase in which reverse-shock-driven compression amplifies the magnetic fi…

astro-ph.HE2026

Temporal evolution of the periodic GeV signal from 4FGL J1913.2+0512 and analysis of the SS 433 / W50 lobes

Ömer Faruk Çoban, Diego F. Torres, Jian Li +3

SS 433 is a microquasar whose relativistic jets precess every ~162 days, providing a laboratory for jet-interstellar medium interactions. We present a comprehensive analysis of 16…

astro-ph.HE2025

The dispersion in pulsar -ray efficiency

Daniel Íñiguez-Pascual, Daniele Viganò, Diego F. Torres

The observational efficiency of pulsars, defined as the ratio of the observationally derived isotropic-equivalent luminosity, , where is the average…

astro-ph.HE2025

Synchro-curvature description of γ-ray light curves and spectra of pulsars: concurrent fitting

Daniel Íñiguez-Pascual, Diego F. Torres, Daniele Viganò

We present a concurrent fitting of spectra and light curves of the whole population of detected gamma-ray pulsars. Using a synchro-curvature model we compare our theoretical output…

astro-ph.HE2024★ 3 cited

Spatio-spectral-temporal Modelling of Two Young Pulsar Wind Nebulae

A. Kundu, Jagdish C. Joshi, C. Venter +5

Recent observations of a few young pulsar wind nebulae (PWNe) have revealed their morphologies in some detail. Given the availability of spatio-spectral-temporal data, we use our m…

astro-ph.HE2024

Synchro-curvature description of -ray light curves and spectra of pulsars: global properties

Daniel Íñiguez-Pascual, Diego F. Torres, Daniele Viganò

This work presents a methodological approach to generate realistic -ray light curves of pulsars, resembling reasonably well the observational ones observed by the Fermi-Large Ar…

astro-ph.HE2020★ 29 cited

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…