Abstract :
I will present results of chemo-hydrodynamical simulations of galaxy formation using the algorithm GCD+. This algorithm includes the effects of gravitation, gasdynamics, and radiative cooling, plus a subgrid treatment of star formation, supernovae feedback, and chemical enrichment. The results will focus on the structural, kinematic, and chemical properties of galaxies, their time-evolution, and how they compare with observations.
Keywords :
astrophysical fluid dynamics; galaxies; gravitation; GCD+ algorithm; chemical enrichment; chemodynamical simulations; chemohydrodynamical simulations; galaxy formation; gasdynamics; gravitation; radiative cooling; star formation; supernovae feedback; Chemicals; Computational modeling; Cooling; Feedback; High performance computing; Kinematics;
