activity
20192021
most citedSNR G39.2-0.3, an Hadronic Cosmic Rays Accelerator

15 citations · 39 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2021

Probing the hadronic nature of the gamma-ray emission associated with Westerlund 2

Emma de Ona Wilhelmi, Enrique Mestre, Diego F. Torres +6

Star-forming regions have been proposed as potential Galactic cosmic-ray accelerators for decades. Cosmic ray acceleration can be probed through observations of gamma-rays produced…

astro-ph.HE20211 cited

Prospects for Galactic transient sources detection with the Cherenkov Telescope Array

A. López-Oramas, A. Bulgarelli, S. Chaty +17

Several types of Galactic sources, like magnetars, microquasars, novae or pulsar wind nebulae flares, display transient emission in the X-ray band. Some of these sources have also…

astro-ph.HE20214 cited

Multi-messenger and transient astrophysics with the Cherenkov Telescope Array

Ž. Bošnjak, A. M. Brown, A. Carosi +142

The discovery of gravitational waves, high-energy neutrinos or the very-high-energy counterpart of gamma-ray bursts has revolutionized the high-energy and transient astrophysics co…

astro-ph.HE202114 cited

Probing the hadronic nature of the gamma-ray emission associated with Westerlund 2

Enrique Mestre, Emma de Ona Wilhelmi, Diego F. Torres +6

Star-forming regions have been proposed as potential Galactic cosmic-ray accelerators for decades. Cosmic-ray acceleration can be probed through observations of gamma-rays produced…

astro-ph.HE202015 cited

SNR G39.2-0.3, an Hadronic Cosmic Rays Accelerator

Emma de Ona Wilhelmi, Iurii Sushch, Robert Brose +3

Recent results obtained with gamma-ray satellites have established supernova remnants as accelerators of GeV hadronic cosmic rays. In such processes, CRs accelerated in SNR shocks…

astro-ph.HE20195 cited

Prospects for the characterization of the VHE emission from the Crab Nebula and Pulsar with the Cherenkov Telescope Array

Enrique Mestre, Emma de Oña Wilhelmi, Roberta Zanin +2

The Cherenkov Telescope Array (CTA) will be the next generation instrument for the very high energy gamma-ray astrophysics domain. With its enhanced sensitivity in comparison with…