Figshare· 2025
Stellar, brown dwarf and multiple star properties from a radiation hydrodynamical simulation of star cluster formation
- 291citations
- 2025year
Short summary
A new radiation hydrodynamical simulation of star cluster formation, resolving masses down to a few Jupiter masses, accurately reproduces observed stellar mass functions and brown dwarf ratios, unlike previous barotropic models.
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Astronomy and AstrophysicsPhysics and Astronomy