Salvatore Orlando
0000-0003-2836-540X
107 papers found
Refreshing results…
Clumping of ejecta and accelerated cosmic rays in the evolution of type Ia SNRs
XMM-Newtonevidence of shocked ISM in SN 1006: indications of hadronic acceleration
Role of Ejecta Clumping and Back-reaction of Accelerated Cosmic Rays in the Evolution of Type Ia Supernova Remnants
Post-Flare Ultraviolet Light Curves Explained With Thermal Instability of Loop Plasma
Modelling the 2010 blast wave of the symbiotic-like nova V407 Cygni
X-Ray Emission From Protostellar Jet Hh 154: The First Evidence of a Diamond Shock?
Constraints on the local interstellar magnetic field from non-thermal emission of SN1006
Unveiling the spatial structure of the overionized plasma in the supernova remnant W49B
Mass accretion to young stars triggered by flaring activity in circumstellar discs
Observational constraints on the modelling of SN 1006
Radio, X-ray and γ-ray surface brightness profiles as powerful diagnostic tools for non-thermal SNR shells
Effects of non-uniform interstellar magnetic field on synchrotron X-ray and inverse-Comptonγ-ray morphology of supernova remnants
Multiwavelength diagnostics of accretion in an X-ray selected sample of CTTSs
On the observability of T Tauri accretion shocks in the X-ray band
The Early Blast Wave of the 2010 Explosion of U Scorpii
The origin of the X-ray-emitting plasma in the eastern edge of the Cygnus Loop
Observability and diagnostics in the X-ray band of shock-cloud interactions in supernova remnants
Generation of radiative knots in a randomly pulsed protostellar jet
X-ray emitting MHD accretion shocks in classical T Tauri stars
Predicted $γ$-ray image of SN 1006 due to inverse Compton emission
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