149 citations · 2.4k across the 69 of their papers we have counts for
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Hydrodynamic simulations unravel the progenitor-supernova-remnant connection in SN 1987A
S. Orlando, M. Ono, S. Nagataki +8
(Abridged) We aim at linking the dynamical and radiative properties of the remnant of SN 1987A to the geometrical and physical characteristics of the parent aspherical SN explosion…
Effects of Radiation in Accretion Regions of Classical T Tauri Stars: Pre-heating of accretion column in non-LTE regime
Salvatore Colombo, Laurent Ibgui, Salvatore Orlando +8
Models and observations indicate that the impact of matter accreting onto the surface of young stars produces regions at the base of accretion columns, in which optically thin and…
Non-LTE radiation hydrodynamics in PLUTO
Salvatore Colombo, Laurent Ibgui, Salvatore Orlando +5
Modeling the dynamics of most astrophysical structures requires an adequate description of the radiation-matter interaction. Several numerical (magneto)hydrodynamics codes were upg…
A new view of the corona of classical T Tauri stars: Effects of flaring activity in circumstellar disks
Salvatore Colombo, Salvatore Orlando, Giovanni Peres +5
Classical T Tauri stars (CTTSs) are young low-mass stellar objects accreting mass from their circumstellar disks. They are characterized by high levels of coronal activity as revea…
Collisionless shock heating of heavy ions in SN 1987A
Marco Miceli, Salvatore Orlando, David N. Burrows +6
Astrophysical shocks at all scales, from those in the heliosphere up to the cosmological shock waves, are typically "collisionless", because the thickness of their jump region is m…