57 citations · 412 across the 22 of their papers we have counts for
22 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…
Predicting the time variation of radio emission from MHD simulations of a flaring T-Tauri star
C. O. G. Waterfall, P. K. Browning, G. A. Fuller +3
We model the time dependent radio emission from a disk accretion event in a T-Tauri star using 3D, ideal magnetohydrodynamic simulations combined with a gyrosynchrotron emission an…
Post-adiabatic supernova remnants in an interstellar magnetic field: oblique shocks and non-uniform environment
O. Petruk, T. Kuzyo, S. Orlando +5
We present very-high-resolution 1D MHD simulations of the late-stage supernova remnants (SNR). In the post-adiabatic stage the magnetic field has an important and significant dynam…
Radio polarization maps of shell-type SNRs II. Sedov models with evolution of turbulent magnetic field
O. Petruk, R. Bandiera, V. Beshley +2
Polarized radio emission has been mapped with great detail in several Galactic supernova remnants (SNRs), but has not yet been exploited to the extent it deserves. We have develope…
Magnetic shuffling of coronal downdrafts
A. Petralia, F. Reale, S. Orlando
Channelled fragmented downflows are ubiquitous in magnetized atmospheres, and have been recently addressed from an observation after a solar eruption. We study the possible back-ef…
XMM-Newton observation of the supernova remnant Kes 78 (G32.8-0.1): Evidence for shock-cloud interaction
M. Miceli, A. Bamba, S. Orlando +4
The Galactic supernova remnant Kes 78 is surrounded by dense molecular clouds, whose projected position overlaps with the extended HESS gamma-ray source HESS J1852-000. The X-ray e…