128 citations · 787 across the 17 of their papers we have counts for
15 papers
Modeling particle acceleration and non-thermal emission in supernova remnants
S. Orlando, M. Miceli, S. Ustamujic +5
According to the most popular model for the origin of cosmic rays (CRs), supernova remnants (SNRs) are the site where CRs are accelerated. Observations across the electromagnetic s…
The fully developed remnant of a neutrino-driven supernova: Evolution of ejecta structure and asymmetries in SNR Cassiopeia A
S. Orlando, A. Wongwathanarat, H. -T. Janka +5
Abridged. We aim at exploring to which extent the remnant keeps memory of the asymmetries that develop stochastically in the neutrino-heating layer due to hydrodynamic instabilitie…
A stellar flare-coronal mass ejection event revealed by X-ray plasma motions
C. Argiroffi, F. Reale, J. J. Drake +6
Coronal mass ejections (CMEs), often associated with flares, are the most powerful magnetic phenomena occurring on the Sun. Stars show magnetic activity levels up to 10^4 times hig…
EUV flickering of solar coronal loops: a new diagnostic of coronal heating
E. Tajfirouze, F. Reale, G. Peres +1
A previous work of ours found the best agreement between EUV light curves observed in an active region core (with evidence of super-hot plasma) and those predicted from a model wit…
Mass Accretion Processes in Young Stellar Objects: Role of Intense Flaring Activity
S. Orlando, F. Reale, G. Peres +1
According to the magnetospheric accretion scenario, young low-mass stars are surrounded by circumstellar disks which they interact with through accretion of mass. The accretion bui…
Hydrodynamic modelling of ejecta shrapnel in the Vela supernova remnant
M. Miceli, S. Orlando, F. Reale +2
Many supernova remnants (SNRs) are characterized by a knotty ejecta structure. The Vela SNR is an excellent example of remnant in which detached clumps of ejecta are visible as X-r…