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Star-forming environments in smoothed particle magnetohydrodynamics simulations II: re-simulating isolated clumps to determine equivalence of extracted clumps and parent simulations
On the properties and implications of collapse-driven MHD turbulence
Enrique Vázquez-Semadeni, Yue Hu, Siyao Xu, Rubén Guerrero-Gamboa and Alex Lazarian Monthly Notices of the Royal Astronomical Society 530(3) 3431 (2024) https://doi.org/10.1093/mnras/stae1085
The Physical Origin of the Stellar Initial Mass Function
Direct collapse of exceptionally heavy black holes in the merger-driven scenario
Lorenz Zwick, Lucio Mayer, Lionel Haemmerlé and Ralf S Klessen Monthly Notices of the Royal Astronomical Society 518(2) 2076 (2022) https://doi.org/10.1093/mnras/stac3204
Influence of magnetic field and stellar radiative feedback on the collapse and the stellar mass spectrum of a massive star-forming clump
Protostellar collapse simulations in spherical geometry with dust coagulation and fragmentation
Ugo Lebreuilly, Valentin Vallucci-Goy, Vincent Guillet, Maxime Lombart and Pierre Marchand Monthly Notices of the Royal Astronomical Society 518(3) 3326 (2022) https://doi.org/10.1093/mnras/stac3220
Saturation Level of Turbulence in Collapsing Gas Clouds
Dust coagulation and fragmentation in a collapsing cloud core and their influence on non-ideal magnetohydrodynamic effects
Yoshihiro Kawasaki, Shunta Koga and Masahiro N Machida Monthly Notices of the Royal Astronomical Society 515(2) 2072 (2022) https://doi.org/10.1093/mnras/stac1919