activity
20032026
most citedPLUTO: a Numerical Code for Computational Astrophysics

1.6k citations · 2.7k across the 18 of their papers we have counts for

collaborators

19 papers

astro-ph.SR2026

3D simulations of magnetospheric accretion in T Tauri stars: I. Disk truncation, stellar torques, and application to observations

George Pantolmos, Claudio Zanni, Jérôme Bouvier

Young stars accrete material from their circumstellar disk through their magnetosphere and undergo contraction; these two processes impact their rotational evolution. We investigat…

astro-ph.SR2026

On the collimation properties of jets with finite Poynting flux launched from Keplerian accretion discs

Thomas Jannaud, Jonathan Ferreira, Claudio Zanni

It is generally accepted that the launching of astrophysical jets requires a large-scale magnetic field threading a central object (black hole or star) and/or its surrounding accre…

astro-ph.HE2026★ 2 cited

The PLUTO Code on GPUs: Offloading Lagrangian Particle Methods

Alessio Suriano, Stefano Truzzi, Agnese Costa +5

The Lagrangian Particles (LP) module of the PLUTO code offers a powerful simulation tool to predict the non-thermal emission produced by shock accelerated particles in large-scale…

astro-ph.SR2024

Simulations of Protostar-Driven Photoionization in Herbig-Haro Jets

Z. Ahmane, A. Mignone, C. Zanni +2

Recent studies showed that observations of line emission from shocks in YSO jets require a substantial amount of ionization of the pre-shock matter. Photoionization from X-ray emit…

astro-ph.SR2024★ 10 cited

Long period modulation of the classical T Tauri star CI Tau: evidence for an eccentric close-in massive planet at 0.17 au

R. Manick, A. P. Sousa, J. Bouvier +13

Detecting planets within protoplanetary disks around young stars is essential for understanding planet formation and evolution. However, planet detection using the radial velocity…

astro-ph.SR2022★ 17 cited

Magnetic Braking of Accreting T Tauri Stars II: Torque Formulation Spanning Spin-Up and Spin-Down Regimes

Lewis G. Ireland, Sean P. Matt, Claudio Zanni

The magnetic interaction between a classical T Tauri star and its surrounding accretion disk is thought to influence its rotational evolution. We use 2.5D magnetohydrodynamic, axis…