Dimensional argument for the impact of turbulent support on the stellar initial mass function

DOI10.1051/0004-6361/201117285zbMath1260.85037arXiv1109.2780OpenAlexW3105423715WikidataQ68679506 ScholiaQ68679506MaRDI QIDQ4905863

Gilles Chabrier, P. Hennebelle

Publication date: 21 February 2013

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1109.2780

zbMATH Keywords

turbulencestars: formationsstars: luminosity function, mass function

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stability and instability of geophysical and astrophysical flows (76E20)

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