CCD photometry of two young Large Magellanic Cloud clusters - NGC 2004 and 2100

Details CCD photometry of two young Large Magellanic Cloud clusters - NGC 2004 and 2100 CCD photometry of two young Large Magellanic Cloud clusters - NGC 2004 and 2100

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.260..782b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 260, no. 4, p. 782-794.

Physics

Optics

15

Astronomical Photometry, Charge Coupled Devices, Early Stars, Magellanic Clouds, Star Clusters, Calibrating, Cassegrain Optics, Cepheid Variables

Scientific paper

In this paper we present results of CCD UBV photometry of stars in two
young LMC clusters: NGC 2004 and 2100. A comparison of recent CCD
investigations of these clusters shows large zero-point discrepancies.

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