activity
20182021
most citedFrom supernova to supernova remnant: comparison of thermonuclear explosion models

31 citations · 60 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2021

On the origin of the asymmetry of the ejecta structure and explosion of G350.10.3

Tomoya Tsuchioka, Yasunobu Uchiyama, Ryota Higurashi +4

We present X-ray analysis of the ejecta of supernova remnant G350.10.3 observed with Chandra and Suzaku, and clarify the ejecta's kinematics over a decade and obtain a new obser…

astro-ph.HE202031 cited

From supernova to supernova remnant: comparison of thermonuclear explosion models

Gilles Ferrand, Donald C. Warren, Masaomi Ono +6

Progress in the three-dimensional modeling of supernovae (SN) prompts us to revisit the supernova remnant (SNR) phase. We continue our study of the imprint of a thermonuclear explo…

astro-ph.HE202018 cited

Probing the magnetic field in the GW170817 outflow using H.E.S.S. observations

H. E. S. S. Collaboration, :, H. Abdalla +230

The detection of the first electromagnetic counterpart to the binary neutron star (BNS) merger remnant GW170817 established the connection between short -ray bursts and BNS merg…

astro-ph.IM201911 cited

X-ray Study of Spatial Structures in Tycho's Supernova Remnant Using Unsupervised Deep Learning

Hiroyoshi Iwasaki, Yuto Ichinohe, Yasunobu Uchiyama

Recent rapid development of deep learning algorithms, which can implicitly capture structures in high-dimensional data, opens a new chapter in astronomical data analysis. We report…

astro-ph.HE2018

Population study of Galactic supernova remnants at very high -ray energies with H.E.S.S.

H. E. S. S. Collaboration, :, H. Abdalla +252

Shell-type supernova remnants (SNRs) are considered prime candidates for the acceleration of Galactic cosmic rays (CRs) up to the knee of the CR spectrum at $\mathrm{E} \approx \ma…