149 citations · 2.4k across the 69 of their papers we have counts for
68 papers
Unraveling the Effects of Dense Medium on a Near to Bohm-Limit Acceleration in Kepler's SNR
Vincenzo Sapienza, Marco Miceli, Oleh Petruk +4
The maximum energy of electrons accelerated by supernova remnants (SNR) is typically limited by radiative losses. In this scenario, the synchrotron cooling time scale is equal to t…
Spatial and dynamical structure of the NGC 2264 star-forming region
E. Flaccomio, G. Micela, G. Peres +7
The processes that lead from molecular clouds to protostars, stellar associations, and the evolution of both, are active research topics. The target of this study, NGC2264, is a be…
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…
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…
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…
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…