233 citations · 3.7k across the 79 of their papers we have counts for
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Accounting for the diversity in stellar environments
Michael Küffmeier, Troels Haugbølle, Åke Nordlund
Stars and their corresponding protoplanetary disks form in diverse environments. To account for these natural variations, we investigate the formation process around nine solar mas…
Episodic accretion: the interplay of infall and disc instabilities
Michael Kuffmeier, Søren Frimann, Sigurd S. Jensen +1
Using zoom-simulations carried out with the adaptive mesh-refinement code RAMSES with a dynamic range of up to we investigate the accretion profil…
Explaining the luminosity spread in young clusters: proto and pre-main sequence stellar evolution in a molecular cloud environment
Sigurd S. Jensen, Troels Haugbølle
Hertzsprung-Russell diagrams of star forming regions show a large luminosity spread. This is incompatible with well-defined isochrones based on classic non-accreting protostellar e…
The stellar IMF from Isothermal MHD Turbulence
Troels Haugbølle, Paolo Padoan, Aake Nordlund
We address the turbulent fragmentation scenario for the origin of the stellar initial mass function (IMF), using a large set of numerical simulations of randomly driven supersonic…
Supernova Driving. IV. The Star Formation Rate of Molecular Clouds
Paolo Padoan, Troels Haugbølle, Åke Nordlund +1
We compute the star formation rate (SFR) in molecular clouds (MCs) that originate {\it ab initio} in a new, higher-resolution simulation of supernova-driven turbulence. Because of…