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A Numerical Study of Galaxy Properties from Cosmological Simulations with Star Formation

G. Yepes·D. Elizondo·Y. Ascasibar
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Abstract

From a set of 3D cosmological simulations which incorporate a self-consistent model of the star-gas interactions, we have been able to obtain a statistically significant sample of galaxy-type halos with observational properties, like colors and luminosities. Using this data-base, we have studied general relations of galaxies, such as the Tully-Fisher relation, luminosity functions, environmental dependences, or cosmic star formation density.

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G. Yepes, D. Elizondo, Y. Ascasibar. 1999-05-31. A Numerical Study of Galaxy Properties from Cosmological Simulations with Star Formation. https://arxiv.org/abs/astro-ph/9905395

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