Image Details

Choose export citation format:

L Dwarfs and the Substellar Mass Function

  • Authors: I. Neill Reid, J. Davy Kirkpatrick, J. Liebert, A. Burrows, J. E. Gizis, A. Burgasser, C. C. Dahn, D. Monet, R. Cutri, C. A. Beichman, and M. Skrutskie

Reid et al. 1999 The Astrophysical Journal 521 613.

  • Provider: AAS Journals

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.

Other Images in This Article
Copyright and Terms & Conditions