Properties and evolution of disk galaxies in a hierarchical formation scenario

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dc.creatorAvila-Reese, V.
dc.creatorFirmani, C.
dc.date2000-09-20
dc.date.accessioned2026-07-07T01:55:32Z
dc.date.available2026-07-07T01:55:32Z
dc.descriptionWe highlight some results from disk galaxy evolution models conceived within a cosmological context. When disk mergers and strong disk-halo feedback are omitted, several properties and correlations of disk galaxies seem to be related to initial conditions given by the CDM model, for example, the intensive galaxy properties, the disk Hubble sequence, and the Tully-Fisher relation in the infrared bands.
dc.description2 pages, to appear in "Galaxy Disks and Disk Galaxies," eds. J. G. Funes & E. M. Corsini (ASP Conference Series)
dc.identifierhttps://arxiv.org/abs/astro-ph/0009315
dc.identifierhttp://arxiv.org/abs/astro-ph/0009315
dc.identifierASP Conference Series, 230, p. 647-648 (2001)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1687
dc.subjectAstrophysics
dc.titleProperties and evolution of disk galaxies in a hierarchical formation scenario
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