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Three UBV sequences in the LMC
Photoelectric and electronographic photometry is presented for threesequences near the clusters NGC 1466, 2214, and 2257. Observations weremade during August 1972-January 1975 with telescopes at Cape Town,Sutherland, and Pretoria. It is found that photoelectric measures ofstars previously observed by Butler (1972) provide a tie to otherphotometric studies.
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Observation and Astrometry data
| Constellation: | Dorado |
| Right ascension: | 06h29m10.30s |
| Declination: | -64°14'14.5" |
| Apparent magnitude: | 8.818 |
| Distance: | 414.938 parsecs |
| Proper motion RA: | -6.6 |
| Proper motion Dec: | 8.9 |
| B-T magnitude: | 8.874 |
| V-T magnitude: | 8.823 |
Catalogs and designations:
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INHABITED SKY
