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A STUDY OF CLUSTERS AND FIELD STARS IN 2 REGIONS IN THE LARGE MAGELLANIC CLOUD .1. CCD PHOTOMETRY IN B AND V
Uppsala universitet.
Uppsala universitet.
Uppsala universitet.
1995 (engelsk)Inngår i: ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, ISSN 0365-0138, Vol. 110, nr 3, s. 533-543Artikkel i tidsskrift (Annet vitenskapelig) Published
Abstract [en]

We present CCD photometry in the Johnson BV system to about V = 23(m) for the stars in six clusters and the surrounding fields in two regions of different nature in the Large Magellanic Cloud. The analysis includes estimations of loss of measured stars du

sted, utgiver, år, opplag, sider
EDITIONS PHYSIQUE , 1995. Vol. 110, nr 3, s. 533-543
Emneord [en]
CATALOGS; MAGELLANIC CLOUDS; GALAXIES; STELLAR CONTENT; FAINT STAR; POPULATION; BAR
Identifikatorer
URN: urn:nbn:se:uu:diva-85401OAI: oai:DiVA.org:uu-85401DiVA, id: diva2:113309
Merknad
Addresses: LINDE P, LUND OBSERV, BOX 43, S-22100 LUND, SWEDEN. MT STROMLO & SIDING SPRING OBSERV, WESTON, ACT 2611, AUSTRALIA. UNIV UPPSALA, ASTRON OBSERV, S-75120 UPPSALA, SWEDEN.Tilgjengelig fra: 2008-10-17 Laget: 2008-10-17 Sist oppdatert: 2011-01-15

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