Hunting for anti-solar differentially rotating stars using the Rossby number. An application to the Kepler field
Context. Anti-solar differential rotation profiles have been found for decades in numerical simulations of convective envelopes of solar-type stars. These profiles are characterized by a slow equator and fast poles (i.e., reversed with respect to the Sun) and have been found in simulations for high Rossby numbers. Rotation profiles like this have
Noraz, Q. et al.
Fecha de publicación:
11
2022