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Effective Star Formation Rates for Cosmological Applications

Marco Spaans·Marcella Carollo
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Abstract

Effective star formation rates in tabular form are computed which yield a prescription for the star formation activity in model galaxies as a function of ambient density, metallicity, and stellar feedback. The effects of supernova explosions on the thermal balance of the Interstellar Medium (ISM) and the presence of a multi-phase ISM are explicitly included. The resulting grid of models can be implemented easily in N-body codes for the computation of star formation processes in merging galaxies and cosmological simulations.

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Marco Spaans, Marcella Carollo. 1998-02-27. Effective Star Formation Rates for Cosmological Applications. https://doi.org/10.1086/305944

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