COYOTES III: observational evidence for a lower limit to the rotational velocity of ZAMS G and K dwarfs.
In order to provide additional constraints to current models of angular momentum evolution of solar-type stars, we have conducted a period-determination program in the Alpha Perseus cluster. We have selected a sample of 22 Alpha Persei G and K dwarfs on the basis of their seemingly slow rotation rate (vsini
Bouvier, J. et al.
Fecha de publicación:
10
1996