52 citations · 60 across the 8 of their papers we have counts for
8 papers
The electron temperature distribution and the high ionization just behind the shock in the Cygnus Loop
Masahiro Ichihashi, Aya Bamba, Dai Tateishi +6
The physical processes behind astrophysical collisionless shocks, such as thermal relaxation and ionization after shock passage, remain poorly understood. To investigate these proc…
Ideas and Requirements for the Global Cosmic-Ray Observatory (GCOS)
Markus Ahlers, Ingo Allekotte, Jaime Alvarez-Muniz +136
After a successful kick-off meeting in 2021. two workshops in 2022 and 2023 on the future Global Cosmic-Ray Observatory (GCOS) focused mainly on a straw man design of the detector…
Two-component jet model for the afterglow emission of GRB 201216C and GRB 221009A and implications for jet structure of very-high-energy gamma-ray bursts
Yuri Sato, Kohta Murase, Yutaka Ohira +2
In recent years, afterglow emission in the very-high-energy (VHE) band above 100 GeV has been clearly detected for at least five gamma-ray bursts (GRBs 180720B, 190114C, 190829A, 2…
Observational constraints on the maximum energies of accelerated particles in supernova remnants
Hiromasa Suzuki, Aya Bamba, Ryo Yamazaki +1
Supernova remnants (SNRs) are thought to be the most plausible sources of Galactic cosmic rays. One of the principal questions is whether they are accelerating particles up to the…
Suzaku and Fermi view of the supernova remnant 3C 396
Aytap Sezer, Tulun Ergin, Nergis Cesur +4
3C 396 is a composite supernova remnant (SNR), consisting of a central pulsar wind nebula (PWN) and a bright shell in the west, which is known to be interacting with molecular clou…
Simulating Cherenkov Telescope Array observation of RX J1713.7-3946
T. Nakamori, H. Katagiri, H. Sano +29
We perform simulations of Cherenkov Telescope Array (CTA) observations of a young supernova remnant RX J1713.7-3946. This target is not only one of the brightest sources ever disco…
Production cross sections of gamma-rays, electrons, and positrons in p-p collisions
T. Shibata, Y. Ohira, K. Kohri +1
Because the production cross sections of gamma-rays, electrons, and positrons made in p-p collisions, and , respectively, are kinem…
Relativistic Electron Shock Drift Acceleration in Low Mach Number Galaxy Cluster Shocks
Shuichi Matsukiyo, Yutaka Ohira, Ryo Yamazaki +1
An extreme case of electron shock drift acceleration in low Mach number collisionless shocks is investigated as a plausible mechanism of initial acceleration of relativistic electr…