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The influence of the cloud virial parameter on the initial mass function
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Wide-binary eccentricity distribution in young star clusters: dependence on the binary separation and mass
The role of the turbulence driving mode for the initial mass function
Sajay Sunny Mathew, Christoph Federrath and Amit Seta Monthly Notices of the Royal Astronomical Society 518(4) 5190 (2022) https://doi.org/10.1093/mnras/stac3415
On the origin of magnetic fields in stars – II. The effect of numerical resolution
James Wurster, Matthew R Bate, Daniel J Price and Ian A Bonnell Monthly Notices of the Royal Astronomical Society 511(1) 746 (2022) https://doi.org/10.1093/mnras/stac123
The IMF and multiplicity of stars from gravity, turbulence, magnetic fields, radiation, and outflow feedback
From the CMF to the IMF: beyond the core-collapse model
V-M Pelkonen, P Padoan, T Haugbølle and Å Nordlund Monthly Notices of the Royal Astronomical Society 504(1) 1219 (2021) https://doi.org/10.1093/mnras/stab844
Strong dependence of the physical properties of cores on spatial resolution in observations and simulations
Galaxy evolution: modelling the role of non-thermal pressure in the interstellar medium
Yuval Birnboim, Shmuel Balberg and Romain Teyssier Monthly Notices of the Royal Astronomical Society 447(4) 3678 (2015) https://doi.org/10.1093/mnras/stu2717
Formation of Prestellar Cores via Non-Isothermal Gas Fragmentation
The relation between accretion rates and the initial mass function in hydrodynamical simulations of star formation
Th. Maschberger, I. A. Bonnell, C. J. Clarke and E. Moraux Monthly Notices of the Royal Astronomical Society 439(1) 234 (2014) https://doi.org/10.1093/mnras/stt2403
THE MATRYOSHKA RUN: A EULERIAN REFINEMENT STRATEGY TO STUDY THE STATISTICS OF TURBULENCE IN VIRIALIZED COSMIC STRUCTURES
Importance of the initial conditions for star formation - I. Cloud evolution and morphology
Philipp Girichidis, Christoph Federrath, Robi Banerjee and Ralf S. Klessen Monthly Notices of the Royal Astronomical Society 413(4) 2741 (2011) https://doi.org/10.1111/j.1365-2966.2011.18348.x
Dimensional argument for the impact of turbulent support on the stellar initial mass function