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New UBVRI photometry for 900 supergiants
A description is presented of the results obtained in connection with asystematic program of supergiant photometry on the Johnson UBVRI system.During the eight years after the start of the program, almost 1000 starshave been observed, about 400 three or more times each. The originalselection of stars used the spectral type catalog of Jaschek et al.(1964) to choose supergiants. Since observations were possible from bothChile and Canada, no declination limits were imposed, and no particularselection criteria were imposed other than to eliminate carbon stars.These are so red as to require enormous extrapolations of thetransformation equations.
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Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1974AJ.....79..682H&db_key=AST
| Mesures d'étoiles doubles effectuées au télescope de 80 cm. de l'Observatoire de Marseille
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Observation and Astrometry data
| Constellation: | わし座 |
| Right ascension: | 19h06m10.76s |
| Declination: | -09°37'56.0" |
| Apparent magnitude: | 6.666 |
| Distance: | 694.444 parsecs |
| Proper motion RA: | 3.7 |
| Proper motion Dec: | -9.6 |
| B-T magnitude: | 7.958 |
| V-T magnitude: | 6.773 |
Catalogs and designations:
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