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Table 9:

Comparison of our model predictions with previous studies.

Study 		\ensuremath {\varepsilon } Indi Ba $T_{\rm {eff}}$ \ensuremath {\varepsilon } Indi Bb $T_{\rm {eff}}$
Smith et al. (2003) 1400,1600 ...
Roellig et al. (2004) 1250 800
Sterzik et al. (2005) 1100 ...
Mainzer et al. (2007) 1250 800
Kasper et al. (2009) 1250-1300 875-925
This work (atm. models) 1300-1340 880-940
This work (evo. models) 1352-1385 976-1011

The last two entries show the determinations of the effective temperatures of the two T dwarfs from this work, both from fitting atmospheric models to the observed spectra, and by comparing the derived luminosities and dynamical system mass with evolutionary models.


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