Rotational evolution of low-mass stars at different metallicities

A lot of efforts have been made recently in understanding the rotational evolution of low-mass stars. However, modelling stars of different clusters at different ages suggests at least slightly different chemical composition. These become even bigger if one aims at studying the whole Kepler field. We investigate here the effects of a variation of chemical composition through metallicity (-1.0 < [Fe/H] < +0.3) on the rotation period evolution of low-mass stars (0.2 - 1.5 M⊙ )