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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

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Showing astro-ph.SRShow all

28 papers · 1 filter

astro-ph.SR2024★ 16 cited

Mixing is easy: New insights for cosmochemical evolution from pre-stellar core collapse

Asmita Bhandare, Benoît Commerçon, Guillaume Laibe +5

Signposts of early planet formation are ubiquitous in substructured young discs. Dense, hot and high-pressure regions formed during gravitational collapse process, integral to star…

astro-ph.SR2024★ 12 cited

Formation of low mass protostars and their circumstellar disks

Adnan Ali Ahmad, Matthias González, Patrick Hennebelle +1

The birth process of circumstellar disks remains poorly constrained due to observational and numerical challenges. Recent numerical works have shown that the small-scale physics, o…

astro-ph.SR2023★ 1 cited

Synthetic populations of protoplanetary disks. Impact of magnetic fields and radiative transfer

U. Lebreuilly, P. Hennebelle, T. Colman +10

Protostellar disks are the product of angular momentum conservation during the protostellar collapse. Understanding their formation is crucial because they are the birthplace of pl…

astro-ph.SR2023★ 23 cited

The birth and early evolution of a low mass protostar

Adnan Ali Ahmad, Matthias González, Patrick Hennebelle +1

Understanding the collapse of dense molecular cloud cores to stellar densities and the subsequent evolution of the protostar is of importance to model the feedback effects such an…

astro-ph.SR2023★ 18 cited

The role of magnetic fields in the formation of multiple massive stars

R. Mignon-Risse, M. González, B. Commerçon

(Abridged) Context. Most massive stars are located in multiple stellar systems. Magnetic fields are believed to be essential in the accretion and ejection processes around single m…

astro-ph.SR2023★ 10 cited

Disk fragmentation around a massive protostar: a comparison of two three-dimensional codes

Raphaël Mignon-Risse, André Oliva, Matthias González +2

(Abridged) Most massive stars are located in multiple systems. The modeling of disk fragmentation, a possible mechanism leading to stellar multiplicity, relies on parallel 3D simul…