395 citations · 3.3k across the 129 of their papers we have counts for
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Polarized radio emission unveils the structure of the pre-supernova circumstellar magnetic field and the radio emission in SN1987A
O. Petruk, V. Beshley, S. Orlando +7
The detected polarized radio emission from remnant of SN1987A opens the possibility to unveil the structure of the pre-supernova magnetic field in the circumstellar medium. Propert…
The supernova remnant SN 1006 as a Galactic particle accelerator
Roberta Giuffrida, Marco Miceli, Damiano Caprioli +6
The origin of cosmic rays is a pivotal open issue of high-energy astrophysics. Supernova remnants are strong candidates to be the Galactic factory of cosmic rays, their blast waves…
Investigating particle acceleration dynamics in interpenetrating magnetized collisionless super-critical shocks
W. Yao, A. Fazzini, S. N. Chen +9
Colliding collisionless shocks appear in a great variety of astrophysical phenomena and are thought to be possible sources of particle acceleration in the Universe. We have previou…
A spatially resolved study of hard X-ray emission in Kepler's SNR: indications of different regimes of particle acceleration
Vincenzo Sapienza, Marco Miceli, Aya Bamba +6
Synchrotron X-ray emission in young supernova remnants (SNRs) is a powerful diagnostic tool to study the population of high energy electrons accelerated at the shock front and the…
High energy gamma-ray detection of supernova remnants in the Large Magellanic Cloud
R. Campana, E. Massaro, F. Bocchino +3
We present the results of a cluster search in the gamma-ray sky images of the Large Magellanic Cloud (LMC) region by means of the Minimum Spanning Tree (MST) and DBSCAN algorithms,…
Additional evidence for a pulsar wind nebula in the heart of SN 1987A from multi-epoch X-ray data and MHD modeling
Emanuele Greco, Marco Miceli, Salvatore Orlando +9
Since the day of its explosion, supernova (SN) 1987A has been closely monitored to study its evolution and to detect its central compact relic. In fact, the formation of a neutron…
Particle energization in colliding subcritical collisionless shocks investigated in the laboratory
A. Fazzini, W. Yao, K. Burdonov +16
Colliding collisionless shocks appear in a great variety of astrophysical phenomena and are thought to be possible sources of particle acceleration in the Universe. To investigate…
Evidence for past interaction with an asymmetric circumstellar shell in the young SNR Cassiopeia A
S. Orlando, A. Wongwathanarat, H. -T. Janka +8
Observations of the SNR Cassiopeia A (Cas A) show asymmetries in the reverse shock that cannot be explained by models describing a remnant expanding through a spherically symmetric…
Negative and Positive Feedback from a Supernova Remnant with SHREC: A detailed Study of the Shocked Gas in IC443
G. Cosentino, I. Jiménez-Serra, J. C. Tan +20
Supernova remnants (SNRs) contribute to regulate the star formation efficiency and evolution of galaxies. As they expand into the interstellar medium (ISM), they transfer vast amou…