All Tables

Table 1: Methods used to estimate the effective temperature scale for the B0.5-1.5 spectral-types.
Table 2: Stars that have been excluded from the analysis. Objects later than B8 are not listed and can be identified from Paper I.
Table 3: Our distance and age estimates together with selected values from the literature.
Table 4: The mean cluster radial velocities ( $v_{\rm r}$ ), cluster centres and radii (see text for details).
Table 5: Johnson UBV colours deduced from the TLUSTY spectra.
Table 6: The mean projected rotational velocities for our higher gravity targets ( $\log~g \geq 3.9$ ; designated "High gravity'') and our apparently evolved targets excluding known supergiants ( $\log~g < 3.9$ ; designated "Low gravity''). The number of stars in each sample is given by n.