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Hydrodynamical simulations of cosmic structures

Hydrodynamical simulations of cosmic structures

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Simulating galaxies<br />

Galaxy astrophysics:<br />

Sub-resolution<br />

star formation and<br />

SN feedback<br />

Properties <strong>of</strong><br />

galaxies: size,<br />

morphology, gas<br />

fraction, bar, Tully-<br />

Fisher, Schmidt-<br />

Kennicutt<br />

Baryon fraction<br />

in DM halos<br />

Can we produce<br />

realistic spiral<br />

galaxies?<br />

Murante et al., in prep.

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