2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/14447We have obtained high resolution spectra of $\sim$40 members of M35, determined the Lithium-T$_{\rm{eff}}$ morphology and the distribution of the rotational velocity for G and K stars, and compared them to those of the Pleiades and other well-known open clusters.4 Pages. Contribution to "Stellar Clusters and Association: Convection, Rotation, and Dynamos", ASP Conf. Series, in pressAstrophysicstext