We compare the absolute visual magnitude of the majority of bright O stars in the sky as predicted from their spectral type with the absolute magnitude calculated from their apparent magnitude and the Hipparcos parallax. We find that many stars appear to be much fainter than expected, up to five magnitudes. We find no evidence for a correlation between magnitude differences and the stellar rotational velocity as suggested for OB stars by Lamers et al. (1997A&A...325L..25L), whose small sample of stars is partly included in ours.

Cone search capability for table J/A+A/428/149/table1 (Characteristics of the O star sample.)

Cone search capability for table J/A+A/428/149/table2 (Characteristics of the B stars in the sample of Lamers et al., 1997A&A...325L..25L depicted in Fig. 5.)