activity
20082019
most citedOptical Albedo Theory of Strongly-Irradiated Giant Planets: The Case of HD 209458b

98 citations · 587 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2019★ 12 cited

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…

astro-ph.IM2019★ 9 cited

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…

astro-ph.SR2019★ 17 cited

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…

astro-ph.SR2014★ 52 cited

Origin of the wide-angle hot H2 in DG Tauri: New insight from SINFONI spectro-imaging

Vanessa Agra-Amboage, S. Cabrit, C. Dougados +3

We wish to test the origins proposed for the extended hot H2 at 2000K around the atomic jet from the T Tauri star DGTau, in order to constrain the wide-angle wind structure and the…

astro-ph.SR2013★ 46 cited

Radiative accretion shocks along nonuniform stellar magnetic fields in classical T Tauri stars

S. Orlando, R. Bonito, C. Argiroffi +9

(abridged) AIMS. We investigate the dynamics and stability of post-shock plasma streaming along nonuniform stellar magnetic fields at the impact region of accretion columns. We stu…

astro-ph.SR2013★ 47 cited

YSO accretion shocks: magnetic, chromospheric or stochastic flow effects can suppress fluctuations of X-ray emission

T. Matsakos, J. -P. Chièze, C. Stehlé +9

Context. Theoretical arguments and numerical simulations of radiative shocks produced by the impact of the accreting gas onto young stars predict quasi-periodic oscillations in the…