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

(2) Instituto de Astronomia y Fisica del Espacio; (3) University of British Columbia; Argentina; A. Saiz (1); Buenos Aires; Canada); Madrid; P. B. Tissera (2); R. Dominguez-Tenreiro (1); S. Courteau (3) ((1) Universidad Autonoma de Madrid

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

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arxiv astro-ph/0101489 v1 pith:E5FUH7AT submitted 2001-01-26 astro-ph

A. Saiz (1) , R. Dominguez-Tenreiro (1) , P. B. Tissera (2) , S. Courteau (3) ((1) Universidad Autonoma de Madrid , Madrid , Spain , (2) Instituto de Astronomia y Fisica del Espacio , Buenos Aires

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Argentina (3) University of British Columbia Vancouver Canada)

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keywords propertiescomparisondatasimulationsagreementalgorithmanalyzeconsistent

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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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