188 citations · 2.2k across the 80 of their papers we have counts for
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Hydrodynamic Modeling of Accretion Impacts in Classical T Tauri Stars: Radiative Heating of the Pre-shock Plasma
G. Costa, S. Orlando, G. Peres +2
Context. It is generally accepted that, in Classical T Tauri Stars, the plasma from the circumstellar disc accretes onto the stellar surface with free fall velocity, and the impact…
Formation of X-ray emitting stationary shocks in magnetized protostellar jets
S. Ustamujic, S. Orlando, R. Bonito +3
X-ray observations of protostellar jets show evidence of strong shocks heating the plasma up to temperatures of a few million degrees. In some cases, the shocked features appear to…
Modeling the shock-cloud interaction in SN 1006: unveiling the origin of nonthermal X-ray and gamma-ray emission
Marco Miceli, Salvatore Orlando, Victor Pereira +9
The supernova remnant SN 1006 is a source of high-energy particles and its southwestern limb is interacting with a dense ambient cloud, thus being a promising region for gamma-ray…
Gaia-ESO Survey: Gas dynamics in the Carina Nebula through optical emission lines
F. Damiani, R. Bonito, L. Magrini +28
We present observations from the Gaia-ESO Survey in the lines of H, [N II], [S II] and He I of nebular emission in the central part of the Carina Nebula. We investigate the prop…
Modeling non-thermal emission from stellar bow shocks
V. Pereira, J. López-Santiago, M. Miceli +2
Runaway O- and early B-type stars passing throughout the interstellar medium at supersonic velocities and characterized by strong stellar winds may produce bow shocks that can serv…
The Gaia-ESO Survey: membership and Initial Mass Function of the Gamma Velorum cluster
L. Prisinzano, F. Damiani, G. Micela +23
Understanding the properties of young open clusters, such as the Initial Mass Function (IMF), star formation history and dynamic evolution, is crucial to obtain reliable theoretica…