Spin-up of low-mass classical bulges in barred galaxies
Secular evolution is one of the key routes through which galaxies evolve along the Hubble sequence. Not only does the disc undergo morphological and kinematic changes, but a pre-existing classical bulge may also be dynamically changed by the secular processes driven primarily by the bar. We study the influence of a growing bar on the dynamical
Saha, Kanak et al.
Fecha de publicación:
3
2012