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Four-colour UVBY and H-beta photometry of all stars earlier than G0 and brighter than MPG of about 10.7 M in Selected Area 203 towards the Chamaeleon-Musca dark clouds
Results are presented of Stromgren uvby(beta) photometry for 213 starsearlier than G0 and brigher than mpg of about 10.7 m inSelected Area 203. The observed area lies close to the geometric centerof the Chamaeleon-Musca dark clouds complex. The results yield V, (b-y),m1, c1, and beta on the standard systems, withoverall rms errors for one observation of one star of 0.010, 0.004,0.007, 0.009, and 0.011, respectively.
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| UBV(RI)c photometry of some standard sequences in the Harvard F regions and in the Magellanic Clouds
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1988MNRAS.231.1047M&db_key=AST
| Standard Stars for VRI Photometry with S25 Response Photocathodes
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Observation and Astrometry data
| Constellation: | Musca |
| Right ascension: | 12h17m06.57s |
| Declination: | -73°32'02.1" |
| Apparent magnitude: | 8.661 |
| Distance: | 763.359 parsecs |
| Proper motion RA: | -14 |
| Proper motion Dec: | -3.7 |
| B-T magnitude: | 8.727 |
| V-T magnitude: | 8.667 |
Catalogs and designations:
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