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Physical parameters of stars in the Scorpio-Centaurus OB association
Walraven photometry is presented of established and probable members ofthe Scorpio-Centaurus OB association. For each star, effectivetemperature and surface gravity are derived using Kurucz (1979)atmosphere models. From the Straizys and Kuriliene (1981) tables,absolute magnitudes are calculated. Distance moduli and visualextinctions are determined for all stars. From a comparison of theHR-diagrams of the stars in each subgroup with theoretical isochrones,the ages of the three subgroups are derived. The distances to the threesubgroups are shown to be different; there is a general trend (alsowithin each subgroup) for the distances to be larger at higher galacticlongitudes. The visual extinction in the youngest subgroupUpper-Scorpius, is well correlated with the IRAS 100-micron map. Thedistance toward the Ophiuchus dark clouds is found to be 125 pc, basedon the photometric distances to the stars. Most of the early-type starsin Upper-Scorpius are located at the far side of the dark clouds.
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Member of following groups:
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Observation and Astrometry data
| Constellation: | Bouvier |
| Right ascension: | 13h54m45.14s |
| Declination: | +20°08'07.1" |
| Apparent magnitude: | 9.509 |
| Proper motion RA: | -23.8 |
| Proper motion Dec: | 31.4 |
| B-T magnitude: | 9.993 |
| V-T magnitude: | 9.549 |
Catalogs and designations:
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