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Properties of Galaxy Disks in Hierarchical Hydrodynamical Simulations: Comparison with Observational Data

A. Saiz·R. Dominguez-Tenreiro·P. B. Tissera·S. Courteau
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Abstract

We analyze the structural and dynamical properties of disk-like objects formed in fully consistent cosmological simulations with an inefficient star formation algorithm. Comparison with data of similar observable properties of spiral galaxies gives satisfactory agreement.

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A. Saiz, R. Dominguez-Tenreiro, P. B. Tissera, S. Courteau. 2001-01-26. Properties of Galaxy Disks in Hierarchical Hydrodynamical Simulations: Comparison with Observational Data. https://arxiv.org/abs/astro-ph/0101489

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