Kavli Affiliate: David Charbonneau | First 5 Authors: Emily K. Pass, David Charbonneau, David W. Latham, Perry Berlind, Michael L. Calkins | Summary: Fully convective M dwarfs typically remain rapidly rotating and magnetically active for billions of years, followed by an abrupt and mass-dependent transition to slow rotation and quiescence. A robust understanding of this […]
Continue.. The Mass Dependence of Hα Emission and Stellar Spindown for Fully Convective M Dwarfs