268 citations · 4.4k across the 75 of their papers we have counts for
7 papers · 2 filters
Diffuse γ-ray emission from self-confined cosmic rays around Galactic sources
M. D'Angelo, G. Morlino, E. Amato +1
The propagation of particles accelerated at supernova remnant shocks and escaping the parent remnants is likely to proceed in a strongly non-linear regime, due to the efficient sel…
Cherenkov Telescope Array Contributions to the 35th International Cosmic Ray Conference (ICRC2017)
F. Acero, B. S. Acharya, V. Acín Portella +1137
List of contributions from the Cherenkov Telescope Array Consortium presented at the 35th International Cosmic Ray Conference, July 12-20 2017, Busan, Korea.
Contribution to diffuse gamma-ray emission coming from self-confined CRs around their Galactic sources
G. Morlino, M. D'Angelo, P. Blasi +1
Recent observations of the diffuse Galactic gamma-ray emission by the Fermi-LAT satellite have shown significant deviations from models which assume the same diffusion properties f…
Pulsar wind nebulae with bow shocks: non-thermal radiation and cosmic ray leptons
A. M. Bykov, E. Amato, A. E. Petrov +2
Pulsars with high spin-down power produce relativistic winds radiating a fraction of the power in the range from radio to gamma-rays in the pulsar wind nebulae (PWNe). The rest of…
Cosmic Ray Transport in the Galaxy: a Review
Elena Amato, Pasquale Blasi
The physics of energetic particle propagation in magnetised environments plays a crucial role in both the processes of acceleration and transport of cosmic rays. Recent theoretical…
Prospects for CTA observations of the young SNR RX J1713.7-3946
The CTA Consortium, :, F. Acero +381
We perform simulations for future Cherenkov Telescope Array (CTA) observations of RX~J1713.73946, a young supernova remnant (SNR) and one of the brightest sources ever discovere…
Modelling Jets, Tori and Flares in Pulsar Wind Nebulae
Oliver Porth, Rolf Buehler, Barbara Olmi +5
In this contribution we review the recent progress in the modeling of Pulsar Wind Nebulae (PWN). We start with a brief overview of the relevant physical processes in the magnetosph…