Gravity or turbulence? VII. The Schmidt-Kennicutt law, the star formation efficiency, and the mass density of clusters from gravitational collapse rather than turbulent support

Manuel Zamora-Aviles, Vianey Camacho, Javier Ballesteros-Paredes +7

We explore the Schmidt-Kennicutt (SK) relations and the star formation efficiency per free-fall time (${\epsilon }_{\mathrm{ff}}$), mirroring observational studies, in numerical simulations of fi…