2 papers
astro-ph.SR2026
How plasma coupling and convective-zone depth shape the rotation of solar-mass stars
Ana Brito, IlÃdio Lopes
Stellar rotation on the main sequence is a complex function of mass and age, displaying multiple regimes whose physical origin remains only partially understood. In particular, the…
astro-ph.SR2024
A study of the electrostatic properties of the interiors of low-mass stars: Possible implications for the observed rotational properties
Ana Brito, IlÃdio Lopes
In the partially ionized material of stellar interiors, the strongest forces acting on electrons and ions are the Coulomb interactions between charges. The dynamics of the plasma a…