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SUMMARY:Modeling the sub-grid side of galaxy formation - Pierluigi Monaco 
 (Trieste)
DTSTART:20141031T113000Z
DTEND:20141031T123000Z
UID:TALK54253@talks.cam.ac.uk
CONTACT:Martin Haehnelt
DESCRIPTION:Hydrodynamical simulations of galaxies have only recently mana
 ged to produce realistic spirals in cosmological dark matter halos. It is 
 widely believed that strong feedback from massive stars is the key to this
  success. I will present simulations run using GADGET3 with a MUlti-Phase 
 Particle Integrator algorithm for star formation and stellar feedback\, ba
 sed on a simple model for the behaviour of the Inter-Stellar Medium at unr
 esolved scales that does not assume the existence of equilibrium solutions
 . I will focus on the quantification of the outflows generated at high red
 shift in our simulations. Results will be used to understand the potential
 ities of our sub-grid model\, the reason for its success\, and some ideas 
 to further challenge such models.\n
LOCATION:Kavli LMR\, IoA
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