All Tables

Table 1: Comparison of the radii of late-type dwarfs measured by the Infrared Flux Method and by interferometry with the theoretical radii of Baraffe et al. (1998) for an age of 10 Gyr and the oberved metalicity. The errors in the observed values are quoted below the appropriate digits.
Table 2: Parameters of least-squares fits of surface brightness vs. V-K or spectral type (see text and footnote on the title page).
Table 3: Intrinsic infrared colors of young disk dwarfs (CIT system).
Table 4: Color m₇₅₀₀-K characterizing the spectral energy distribution of main-sequence stars of luminosity class V (see text).
Table 5: Examples of distances of CVs determined by the surface brightness method. Columns (1) to (4) contain information of the secondary star, Col. (5) the contribution of the secondary star to the observed flux at 7500 Å, Cols. (6) and (7) the V and K-magnitudes of the secondary star, Col. (8) the mass used in calculating the distances $d_{\rm 7500}$ , d_V, and d_K in Cols. (9)-(11), and Col. (12) gives the trigonometric distance if available. See text for errors of the quantities in Cols. (4) to (8).