Chemical Evolution of the Stellar and Gaseous Components of Galaxies in Hydrodynamical Cosmological Simulations

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dc.creatorCora, S. A.
dc.creatorTissera, P. B.
dc.creatorLambas, D. G.
dc.creatorMosconi, M. B.
dc.date2000-10-23
dc.date.accessioned2026-07-07T01:56:11Z
dc.date.available2026-07-07T01:56:11Z
dc.descriptionWe present preliminary results on the effects of mergers on the chemical properties of galactic objects in hierarchical clustering scenarios. We adopt a hydrodynamical chemical code that allows to describe the coupled evolution of dark matter and baryons within a cosmological context. We found that disk-like and spheroid-like objects have distinctive metallicity patterns that may be the result of different evolution.
dc.description2 pages, 1 Postscript figures. Proceeding of Galaxy Disks and Disk Galaxies, Rome, 2000
dc.identifierhttps://arxiv.org/abs/astro-ph/0010462
dc.identifierhttp://arxiv.org/abs/astro-ph/0010462
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1904
dc.subjectAstrophysics
dc.titleChemical Evolution of the Stellar and Gaseous Components of Galaxies in Hydrodynamical Cosmological Simulations
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