Angular momentum evolution for galaxies
  Using cosmological hydrodynamics simulations we study the angular momentum
content of the simulated galaxies in relation with their morphological type. We
found that not only the angular momentum of the disk component follow the
expected theoretical relation, Mo, Mao & Whiye (1998), but also the spheroidal
one, with a gap due to its lost of angular momentum, in agreement with Fall &
Romanowsky (2013),. We also found that the galaxy size can plot in one general
relation, despite the morphological type, as found by Kravtsov (2013).
