How First Hydrostatic Cores, Tidal Forces, and Gravoturbulent Fluctuations Set the Characteristic Mass of Stars
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab3d46/pdf
Reference55 articles.
1. Bondi–Hoyle–Littleton accretion and the upper-mass stellar initial mass function
2. A Universal Stellar Initial Mass Function? A Critical Look at Variations
3. The MLP distribution: a modified lognormal power-law model for the stellar initial mass function
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5. Collapse of a Molecular Cloud Core to Stellar Densities: The First Three-dimensional Calculations
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