Photoelectric UBVRI sequences in the Magellanic Cloud clusters Lindsay 1, NGC 339, NGC 361, and NGC 1466

Details Photoelectric UBVRI sequences in the Magellanic Cloud clusters Lindsay 1, NGC 339, NGC 361, and NGC 1466 Photoelectric UBVRI sequences in the Magellanic Cloud clusters Lindsay 1, NGC 339, NGC 361, and NGC 1466

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aj.....99.1488a&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 99, May 1990, p. 1488-1490.

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5

Astronomical Photometry, Electrophotometry, Magellanic Clouds, Star Clusters, Ubv Spectra, Charge Coupled Devices, Color-Magnitude Diagram, Stellar Evolution, Stellar Luminosity

Scientific paper

UBVRI sequences in three Small Magellanic Cloud (SMC) clusters Lindsay 1, NGC 339, NGC 361, and in NGC 1466, which lies between the two Magellanic Clouds, are presented. These sequences are appropriate for charge-coupled device (CCD) coverage. Only BV standards have been published in NGC 339 and UBV in NGC 1466; no sequences exist for the two other clusters.

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