The local galaxy population is dominated by low B/T (<0.3) systems;at low masses,most of galaxies are "bulgeless" (Weinzirl + 09;Kormendy+ 10;Fisher & Drory 10,1
Schmidt law star formation SFR dependent SN winds satellite gas stripping morphological transformation assembly through mergers
starbursts through mergers Magor
Radiative Transfer.Radiative Transfer ·Radiation field described by intensity function I(x,n,v,t) ·Boltzmann equation:(e)I/(e)t+c/a▽(nI)=(e)I/(e)t|sources-(e