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Effects of star cluster evolution on emission line ratios and the application to H II galaxies - Including a calibration of the R-23 vs. 12+log(O/H) relationship
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Faculty of Science and Technology, Astronomical observatory.
1997 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 321, no 1, 29-44 p.Article in journal (Refereed) Published
Abstract [en]

A model of spectral evolution of star forming galaxies of various metallicity has been used to study the relation between the optical emission line ratio R-23 = ([OII]lambda 3727 +[OIII]lambda lambda 4959,5007)/H beta and the nebular oxygen abundance. It

Place, publisher, year, edition, pages
SPRINGER VERLAG , 1997. Vol. 321, no 1, 29-44 p.
Keyword [en]
galaxies: evolution; galaxies: stellar content; galaxies: starburst; DWARF IRREGULAR GALAXIES; OXYGEN ABUNDANCES; COMPOSITION GRADIENT; THEORETICAL-MODELS; SOUTHERN GALAXIES; HELIUM ABUNDANCE; STELLAR MODELS; CHEMICAL-COMPOSITION; PHYSICAL CONDITIONS; PLA
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-85347OAI: oai:DiVA.org:uu-85347DiVA: diva2:113255
Note
Addresses: Olofsson K, ASTRON OBSERV, BOX 515, S-75120 UPPSALA, SWEDEN.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-15

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