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SYNTHETIC ABSORPTION-LINE STRENGTHS IN STAR-FORMING REGIONS, AND THE EFFECTS ON THE HELIUM ABUNDANCE DETERMINATION
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Faculty of Science and Technology, Astronomical observatory.
1995 (English)In: ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, ISSN 0365-0138, Vol. 111, no 1, 57-73 p.Article in journal (Refereed) Published
Abstract [en]

Spectral evolutionary calculations have been employed in order to follow the behaviour of absorption lines in single-burst star forming regions. The model calculations are based on theoretical evolutionary tracks and model atmosphere stellar spectra at 5

Place, publisher, year, edition, pages
EDITIONS PHYSIQUE , 1995. Vol. 111, no 1, 57-73 p.
Keyword [en]
GALAXIES; EVOLUTION; GALAXIES; STELLAR CONTENT; INTERSTELLAR MEDIUM; HII-REGIONS; LINES; PROFILE STARS; MASS FUNCTION; BLUE COMPACT GALAXIES; M-CIRCLE-DOT; SPECTRAL EVOLUTION; STELLAR MODELS; POPULATIONS; GRIDS
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-85399OAI: oai:DiVA.org:uu-85399DiVA: diva2:113307
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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