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

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dc.creatorSaiz, A.
dc.creatorDominguez-Tenreiro, R.
dc.creatorTissera, P. B.
dc.creatorCourteau, S.
dc.date2001-01-26
dc.date.accessioned2026-07-07T01:57:32Z
dc.date.available2026-07-07T01:57:32Z
dc.descriptionWe 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.
dc.description2 pages, 2 figures. To appear in the Proceedings of the Conference "Galaxy Disks and Disk Galaxies", Rome, 12-16 June 2000
dc.identifierhttps://arxiv.org/abs/astro-ph/0101489
dc.identifierhttp://arxiv.org/abs/astro-ph/0101489
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2423
dc.subjectAstrophysics
dc.titleProperties of Galaxy Disks in Hierarchical Hydrodynamical Simulations: Comparison with Observational Data
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