Image Details
Caption: Fig. 3.
Comparison between the Burrows et al. (1993, 1997) (filled squares) and Baraffe et al. (1998) models (open triangles) in the (log II L, Teff)‐plane. The Burrows et al. data are plotted for masses of 0.02, 0.03, 0.04, 0.05, 0.06, 0.07, 0.075, 0.08, 0.09, 0.1, 0.11, and 0.15 M⊙; the Baraffe et al. data points are for masses of 0.035, 0.045, 0.05, 0.06, 0.070, 0.072, 0.075, 0.08, 0.09, 0.10, 0.13, 0.15, 0.175, 0.20 M⊙ (0.1 Gyr); 0.06 M⊙ et seq. for 1 Gyr; and 0.075 M⊙ et seq. for 10 Gyr.
© 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.