Further evidence of saturated, boosted, and disrupted magnetic braking from evolutionary tracks of cataclysmic variables
Date Issued
2025-04
Author(s) USM
Schreiber, Matthias
Belloni, D.
Departamento de Física
DOI
10.1051/0004-6361/202553757
Abstract
Context. Angular momentum loss through magnetic braking drives the spin-down of low-mass stars and the orbital evolution of a variety of close binary stars. Current theories for magnetic braking, often calibrated for one particular type of system, predict
