Seminar @ DF-AS - P. Mitchell - The physics driving the star formation rates of star-forming galaxies

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Data evento
Data inizio evento: 
29/11/2017 - 11:30
Data fine evento: 
29/11/2017 - 12:30
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It has been recognised for 10 years that the observed evolution of galaxy star formation rates at a given stellar mass does not agree with predictions from models and simulations. I will examine the various physical processes which play a role in these predictions, and argue that current observations imply that the efficiency of feedback must evolve with cosmic time. I will demonstrate different options for how this can be achieved empirically, and conclude by examining the behaviour of the Eagle simulations to see if there is a scenario which is preferred by current hydrodynamical simulations.


Villa Bazzoni

Ultimo aggiornamento: 28-11-2017 - 13:58