activity
20072026
most citedCollapse of massive magnetized dense cores using radiation-magneto-hydrodynamics: early fragmentation inhibition

225 citations · 3.6k across the 72 of their papers we have counts for

collaborators

76 papers

astro-ph.IM2026

Bridging the gap between stars and planets

Aina Palau, Dimitris Stamatellos, Matthew Bate +58

The formation mechanisms of brown dwarfs (BDs) and free-floating planets (FFPs) are poorly constrained. The two main competing scenarios include the star-like scenario, where these…

astro-ph.GA2026

Series of core collapse numerical simulations (SOLANUM) I: Modelling the early and late infall in a sun-like protostar

D. Navarro-Almaida, B. Commerçon, U. Lebreuilly +5

Magnetohydrodynamical simulations and interferometric observations toward young stellar objects reveal the accretion of gas that may alter the physical properties and chemical comp…

astro-ph.GA2026

The dominance of turbulence over magnetism in the formation of massive star cluster seeds

Junhao Liu, Patricio Sanhueza, Piyali Saha +32

High-mass stars form in protoclusters, where gravo-magnetic processes shape collapsing clouds and clumps to be elongated preferentially perpendicular to magnetic (B) fields. Yet it…

astro-ph.GA2025

Two-moment cosmic ray transport in RAMSES

Joki Rosdahl, Yohan Dubois, Benoit Commercon +3

Cosmic rays (CRs) are an important source of feedback in a variety of astrophysical contexts. Magneto-hydrodynamical (MHD) simulations treating CRs as a fluid have shown that how t…

astro-ph.GA2025

The Influence of Magnetic Fields on Second-Generation Star Formation in Globular Clusters

Asiyeh Yaghoobi, Fatemeh Tabatabaei, Joakim Rosdahl +3

We investigate the previously unexplored role of magnetic fields in the formation of second-generation (SG) stars in proto-globular clusters (GCs) using 3D radiation-magnetohydrody…

astro-ph.GA2025

Cosmic ray and plasma coupling for isothermal supersonic turbulence in the magnetized interstellar medium

Matt L. Sampson, James R. Beattie, Romain Teyssier +5

Cosmic rays (CRs) are an integral part of the non-thermal pressure budget in the interstellar medium (ISM) and are the leading-order ionization mechanism in cold molecular clouds.…