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A model of spectral galaxy evolution including the effects of nebular emission
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Department of Physics and Astronomy, Observational Astronomy.
Department of Physics and Astronomy, Observational Astronomy.
Department of Physics and Astronomy, Observational Astronomy.
Department of Physics and Astronomy, Observational Astronomy.
2001 (English)In: ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, Vol. 375, no 3, 814-826 p.Article in journal (Refereed) Published
Abstract [en]

This paper presents a new spectral evolutionary model of galaxies, properly taking the effects of nebular emission and pre-main sequence evolution into account. The impact of these features in different photometric filters is evaluated, along with the inf

Place, publisher, year, edition, pages
2001. Vol. 375, no 3, 814-826 p.
Keyword [en]
galaxies : evolution; galaxies : fundamental parameters; galaxies : ISM; galaxies : stellar content; SURFACE-BRIGHTNESS GALAXIES; LOW-MASS STARS; M-CIRCLE-DOT; GLOBULAR-CLUSTERS; STELLAR MODELS; HORIZONTAL-BRANCH; DWARF GALAXIES; GIANT BRANCH; ELEMENT ABU
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-36672OAI: oai:DiVA.org:uu-36672DiVA: diva2:64571
Note
Addresses: Zackrisson E, Astron Observ, Box 515, S-75120 Uppsala, Sweden. Astron Observ, S-75120 Uppsala, Sweden. Observ Strasbourg, F-67000 Strasbourg, France.Available from: 2008-06-17 Created: 2008-06-17 Last updated: 2011-01-13

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Bergvall, NOlofsson, K

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