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AGN jets do not prevent the suppression of conduction by the heat buoyancy instability in simulated galaxy clusters

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Influence of protostellar jets and HII regions on the formation and evolution of stellar clusters

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Meshless methods for magnetohydrodynamics with vector potential

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Towards convergence of turbulent dynamo amplification in cosmological simulations of galaxies

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Cosmic rays and thermal instability in self-regulating cooling flows of massive galaxy clusters

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A discontinuous Galerkin solver in theflashmultiphysics framework

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B. Commerçon, M. González, R. Mignon-Risse, P. Hennebelle and N. Vaytet
Astronomy & Astrophysics 658 A52 (2022)
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The signature of large-scale turbulence driving on the structure of the interstellar medium

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Dust dynamics in ramses – I. Methods and turbulent acceleration

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Momentum deposition of supernovae with cosmic rays

Francisco Rodríguez Montero, Sergio Martin-Alvarez, Debora Sijacki, et al.
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Shattering and growth of cold clouds in galaxy clusters: the role of radiative cooling, magnetic fields, and thermal conduction

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Exponential Integrators for Resistive Magnetohydrodynamics: Matrix-free Leja Interpolation and Efficient Adaptive Time Stepping

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Physical properties and real nature of massive clumps in the galaxy

Zu-Jia Lu, Veli-Matti Pelkonen, Mika Juvela, et al.
Monthly Notices of the Royal Astronomical Society 510 (2) 1697 (2021)
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Cosmological magnetogenesis: the Biermann battery during the Epoch of reionization

Mara Attia, Romain Teyssier, Harley Katz, Taysun Kimm, Sergio Martin-Alvarez, Pierre Ocvirk and Joakim Rosdahl
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Introducing SPHINX-MHD: the impact of primordial magnetic fields on the first galaxies, reionization, and the global 21-cm signal

Harley Katz, Sergio Martin-Alvarez, Joakim Rosdahl, Taysun Kimm, Jérémy Blaizot, Martin G Haehnelt, Léo Michel-Dansac, Thibault Garel, Jose Oñorbe, Julien Devriendt, Adrianne Slyz, Mara Attia and Romain Teyssier
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A low-dissipation HLLD approximate Riemann solver for a very wide range of Mach numbers

Takashi Minoshima and Takahiro Miyoshi
Journal of Computational Physics 446 110639 (2021)
https://doi.org/10.1016/j.jcp.2021.110639

Collapse of turbulent massive cores with ambipolar diffusion and hybrid radiative transfer

R. Mignon-Risse, M. González and B. Commerçon
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An arbitrary high-order Spectral Difference method for the induction equation

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The role of the halo magnetic field on accretion through high-velocity clouds

Asger Grønnow, Thor Tepper-García, Joss Bland-Hawthorn and Filippo Fraternali
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Collapse of turbulent massive cores with ambipolar diffusion and hybrid radiative transfer

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Strong dependence of the physical properties of cores on spatial resolution in observations and simulations

F. Louvet, P. Hennebelle, A. Men’shchikov, et al.
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Cartesian CFD Methods for Complex Applications

Müller Moreira Lopes, Margarete Oliveira Domingues, Ralf Deiterding and Odim Mendes
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Protoplanetary Disk Birth in Massive Star-forming Clumps: The Essential Role of the Magnetic Field

Ugo Lebreuilly, Patrick Hennebelle, Tine Colman, Benoît Commerçon, Ralf Klessen, Anaëlle Maury, Sergio Molinari and Leonardo Testi
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Spectral index of synchrotron emission: insights from the diffuse and magnetised interstellar medium

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Unravelling the origin of magnetic fields in galaxies

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Monthly Notices of the Royal Astronomical Society 504 (2) 2517 (2021)
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The dynamical state of massive clumps

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Calibrating the Davis–Chandrasekhar–Fermi Method with Numerical Simulations: Uncertainties in Estimating the Magnetic Field Strength from Statistics of Field Orientations

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Production and excitation of molecules by dissipation of two-dimensional turbulence

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Monthly Notices of the Royal Astronomical Society 495 (1) 816 (2020)
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A statistical analysis of dust polarization properties in ALMA observations of Class 0 protostellar cores

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Statistical description of dust polarized emission from the diffuse interstellar medium

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