Fig. 16.
Posterior probability distributions for the density and temperature of the primary star in J0218−31 is shown in the top panel. The zero-age main sequence is show(black-dashed) along with the best fitting isochrone (blue-solid) and the respective isochrones for ±1-σ in [Fe/H]. Lower panels: PPD distributions for M1, M2 and τ with best-fitting double-Gaussian models in red.
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