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On the history of star formation in the bar of the Large Magellanic Cloud
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Faculty of Science and Technology, Astronomical observatory.
1997 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 322, no 2, L13-L16 p.Article in journal (Refereed) Published
Abstract [en]

With the HST PC and uvby photometry, we investigate evolutionary signatures in a field in the centre of the LMC Bar. Field stars close to the turn off point in the HR diagram are used for a study of ages and evolution of the stellar popu lations dominatin

Place, publisher, year, edition, pages
SPRINGER VERLAG , 1997. Vol. 322, no 2, L13-L16 p.
Keyword [en]
Large Magellanic Cloud; stellar evolution; metallicity; luminosity function; uvby photometry; CHEMICAL EVOLUTION; LUMINOSITY FUNCTION; METAL ABUNDANCE; MAIN-SEQUENCE; LMC CLUSTERS; FAINT STAR; SUPERGIANTS; FIELD; REGIONS; COLORS
URN: urn:nbn:se:uu:diva-85343OAI: oai:DiVA.org:uu-85343DiVA: diva2:113251
Addresses: Ardeberg A, LUND OBSERV, BOX 43, S-22100 LUND, SWEDEN. UNIV UPPSALA, ASTRON OBSERV, S-75120 UPPSALA, SWEDEN. AARHUS UNIV, INST PHYS & ASTRON, DK-8000 AARHUS C, DENMARK.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-15

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