Chemical Evolution along the Hubble sequence

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dc.creatorMolla, Mercedes
dc.creatorDiaz, A.
dc.creatorFerrini, Federico
dc.date2001-04-03
dc.date.accessioned2026-07-07T01:58:07Z
dc.date.available2026-07-07T01:58:07Z
dc.descriptionWe show a grid of multiphase models whose results are valid for any spiral galaxy, using as input the luminosity or the rotation velocity and the morphological type, measured by the classical index T from 1 to 10.
dc.description4 pag., 2 figures, contribution to "IV Reunion Cientifica de la SEA"
dc.identifierhttps://arxiv.org/abs/astro-ph/0104046
dc.identifierhttp://arxiv.org/abs/astro-ph/0104046
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2650
dc.subjectAstrophysics
dc.titleChemical Evolution along the Hubble sequence
dc.typetext

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