Dynamical heating of newb
Dynamical heating of newborn stars driven by accretion-induced orbital tightening
Dynamical heating of newborn stars driven by accretion-induced orbital tightening
arXiv:2502.18016v1 Announce Type: new
Abstract: In previous works, we have shown that stars in the Orion and the Lagoon Nebula Clusters, and simulations of collapsing clouds, exhibit constant velocity dispersion as a function of mass, a result described by Lynden-Bell 50 years ago as an effect of a…