The near-IR luminosity-metallicity relationship for dwarf irregular galaxies

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dc.creatorSaviane, Ivo
dc.creatorRiegerbauer, R.
dc.creatorHeld, E. V.
dc.creatorIvanov, V.
dc.creatorAlloin, D.
dc.creatorBresolin, F.
dc.creatorMomany, Y.
dc.creatorRich, R. M.
dc.creatorRizzi, L.
dc.date2003-10-15
dc.date2003-12-06
dc.date.accessioned2026-07-07T02:10:29Z
dc.date.available2026-07-07T02:10:29Z
dc.descriptionWe briefly describe our on-going investigation of the near-IR luminosity-metallicity relationship for dwarf irregular galaxies in nearby groups of galaxies. The motivations of the project and the observational databases are introduced, and a preliminary result is presented. The 12+log(O/H) vs.H plane must be populated with more low-luminosity galaxies before a definite conclusion can be drawn.
dc.descriptionTo be published in "Recycling intergalactic and interstellar matter", IAU Symposium Series, Vol. 217, 2004, Pierre-Alain Duc, Jonathan Braine and Elias Brinks, eds
dc.identifierhttps://arxiv.org/abs/astro-ph/0310438
dc.identifierhttp://arxiv.org/abs/astro-ph/0310438
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6756
dc.subjectAstrophysics
dc.titleThe near-IR luminosity-metallicity relationship for dwarf irregular galaxies
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