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The fundamental physical parameters of main-sequence and near main-sequence B type stars as derived from uvby,beta photometry
From spectrophotometric measurements of hydrogen line intensities, uvbyphotometry and photoelectrically determined H-beta and H-gamma indicesof 75 B2-B6 main-sequence stars, effective temperature and surfacegravity are derived by using the model atmospheres computed by Kurucz(1974). Comparisons between the g values and the MK luminosityclassification show good agreement for the MK standard stars but ratherserious disagreement for the average stars in such a way that most ofthe stars classified in luminosity class V really belong to class IV.Using the evolutionary model sequences calculated by Hejlesen et al.(1972) the stellar mass, age and luminosity are determined from the uvbyand beta data through effective temperature and surface gravity. Thetheoretically derived luminosities are in excellent agreement with theluminosities derived by calibrations.
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Observation and Astrometry data
| Constellation: | Hase |
| Right ascension: | 05h45m09.11s |
| Declination: | -22°15'45.8" |
| Apparent magnitude: | 9.327 |
| Proper motion RA: | 35.5 |
| Proper motion Dec: | 16.1 |
| B-T magnitude: | 10.096 |
| V-T magnitude: | 9.391 |
Catalogs and designations:
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