Toward a galaxian luminosity-metallicity relation spanning ten magnitudes

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dc.creatorSaviane, Ivo
dc.creatorBresolin, Fabio
dc.creatorSalzer, John
dc.date2007-02-01
dc.date.accessioned2026-07-07T07:44:23Z
dc.date.available2026-07-07T07:44:23Z
dc.descriptionWe describe the two projects by which we are assembling a database of near-IR luminosities and direct oxygen abundances for both high- and low-mass star-forming galaxies in the nearby Universe. This will eventually allow us to construct the first reliable and homogeneous luminosity-metallicity relation, to be compared to theoretical models of galactic evolution, and to the relations for galaxies at higher redshifts.
dc.descriptionTo appear in the proceedings of "From Stars to Galaxies: Building the pieces to build up the Universe" (Venice, October 16-20, 2006). ASP Conf. Ser
dc.identifierhttps://arxiv.org/abs/astro-ph/0702041
dc.identifierhttp://arxiv.org/abs/astro-ph/0702041
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/123177
dc.subjectAstrophysics
dc.titleToward a galaxian luminosity-metallicity relation spanning ten magnitudes
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