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Table 1:

Distribution of the sample stars into four Strömgren groups (before parallax selection).

Group
Spectral type Luminosity class $\beta$ Number of stars Calibration
1 B0 to A0 III to V $2.59<\beta<2.88$ 993 Crawford (1978)
2 A0 to A3 III to V $2.87<\beta<2.93$ 626 Hilditch et al. (1983)
3 A3 to F0 III to V $2.72<\beta<2.88$ 1517 Crawford (1979)
4 F0 to G2 III to V $2.56<\beta<2.72$ 3857 Crawford (1975)
TOTAL       6993  


Source LaTeX | All tables | In the text

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