Chemical and Spectrophotometric Evolutionary Models for Emission Line Star-forming Galaxies

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dc.creatorManjón, M. L. Martín
dc.creatorMollá, M.
dc.creatorDíaz, A. I.
dc.creatorTerlevich, R.
dc.date2007-12-04
dc.date.accessioned2026-07-07T08:47:09Z
dc.date.available2026-07-07T08:47:09Z
dc.descriptionWe present a self-consistent model under a star-bursting scenario for H{\sc ii} galaxies, combining different codes of chemical evolution, evolutionary population synthesis and photoionization. The results obtained reproduce simultaneoulsy the observed abundances, diagnostic diagrams and equivalent width-colour relations for local H{\sc ii} galaxies.
dc.description2 pages, 4 figures, proceedings to Formation and Evolution of Galaxy Disks conference, Rome 2007
dc.identifierhttps://arxiv.org/abs/0712.0441
dc.identifierhttp://arxiv.org/abs/0712.0441
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/143499
dc.subjectAstrophysics
dc.titleChemical and Spectrophotometric Evolutionary Models for Emission Line Star-forming Galaxies
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