The BOK and Tifft UBV sequence in the Large Magellanic Cloud Revised and extended

Details The BOK and Tifft UBV sequence in the Large Magellanic Cloud Revised and extended The BOK and Tifft UBV sequence in the Large Magellanic Cloud Revised and extended

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...114..213a&link_type=abstract

Astronomy and Astrophysics, vol. 114, no. 1, Oct. 1982, p. 213-215.

Astronomy and Astrophysics

Astrophysics

5

Magellanic Clouds, Star Clusters, Ubv Spectra, Astronomical Photometry, Photoelectric Emission, Visual Photometry

Scientific paper

A UBVRI photoelectric sequence of 15 stars in the northwestern section of the bar of the Large Magellanic Cloud is presented. Most of these stars, whose V magnitude range is 9.4-15.3, had previously been observed in the UBV by Bok and Bok (1969), and in the BV by Tifft and Snell (1971). The agreement in V and B-V is satisfactory for the cases of both previous investigators, with the exception of stars 10 and 14 in the B-V, where the present values are redder.

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