Figshare· 2025
The Mass-Dependence of Angular Momentum Evolution in Sun-Like Stars
- 225citations
- 2025year
Short summary
A new scaling for stellar-wind torque, incorporating mass and Rossby number, explains why low-mass stars retain rapid rotation longer than sun-like stars and why older low-mass stars rotate slower than older sun-like stars.
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Astronomy and AstrophysicsPhysics and Astronomy