Unified Cloudy Models of M, L, and T Dwarfs  ver.2/addendum 

                              29 Aug. 2015


                                T. Tsuji




   The following sub-directories are added to the ver.2:


    The fully dusty models of case B based on the classical solar C & O 
    abundances (case _a.dat); 

      Ba50   :   Tcr = T0 (case B),    log g = 5.0,  Teff = 2000 - 2600K
        525  :                                 5.25, Teff = 2000 - 2600K
        55   :                                 5.5,  Teff = 2000 - 2600K


    The fully dusty models of case B based on the downward revised solar 
    C & O abundances (case_c.dat); 

      Bc525  :   Tcr = T0 (case B),    log g = 5.25, Teff = 2000 - 2600K
        55   :                                 5.5,  Teff = 2000 - 2600K


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