Fig. 13
Effective temperatures and radii for SW CMa shown as a function of the measured mass, with the observational errors represented by the shaded boxes. They are compared against [Fe/H] = + 0.05 Yonsei-Yale isochrones by Yi et al. (2001) from 500 Myr to 900 Myr, in steps of 100 Myr, with [α/Fe] = 0.0. The best-fitting model is indicated with a heavier line.
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