Nonaxisymmetric models of galaxy velocity maps
Galaxy velocity mapsoften show the typical pattern of a rotating disk, consistent with the dynamical model where emitters rotate in circular orbits around the galactic center. The simplest template used to fit these maps consists in the rotating disk model (RDM) where the amplitude of circular velocities is fixed by the observed velocity profile
Sylos Labini, F. et al.
Fecha de publicación:
2
2019