Variable magnetic field and adaptive mixing-length: reproducing Li abundances and constraining rotational evolution of solar-type stars in clusters

Documenti analoghi

• Kepler main-sequence solar-like stars: surface rotation and magnetic-activity evolution
  di: Santos, A. R. G., et al.
  Pubblicazione: (2024)
• The rotation-magnetism relationship in solar-type stars. Constraining magnetic flux emergence rates
  di: Isik, Emre, et al.
  Pubblicazione: (2025)
• Low-latitude magnetic flux emergence on rapidly rotating solar-type stars
  di: Işık, Emre, et al.
  Pubblicazione: (2024)
• Rotational evolution of slow-rotator sequence stars. II. Modeling the wind braking and the rotational coupling in the entire mass range of solar-like stars
  di: Spada, F., et al.
  Pubblicazione: (2025)
• Wave propagation and transmission in a rotating solar-type star
  di: Xu, Yuru, et al.
  Pubblicazione: (2025)