The "H5_out_co_MWD_TWD_dM/dt_#_mixed# directories contain MPPNP-processed hdf files for CO nova models.
Main model parameters are indicated in the directory name,
where MWD and TWD are the initial WD mass and central temperature, dM/dt is the letter-encoded mass accretion
rate (X corresponds to dM/dt = 2e-10 Msun/yr, and B to dM/dt = 1e-11 Msun/yr), # is the number of models 
in the evolutionary sequence, and "mixed" means that the WD was accreting a mixture of equal amounts (50%) of 
WD and solar-composition materials.

These directories also contain the file with the accreted composition, co_wd_MWD_mixed.ppn, and the file with
the solar composition, Solar_Composition.

In the MPPNP post-processing computations, a list of 147 isotopes, falk_isotopedatabase.txt, has been used.
It is placed in the directory ppd.

A table below gives the maximum mass interval over which the abundances can be averaged in the envelope, and
the range of model numbers that were processed.

   co nova model             Mmin      Mmax      #min  #max

   co_1.0_12_X_650_mixed     1.000000  1.000051  1     600

   co_1.0_20_X_650_mixed     1.000000  1.000021  60    600

   co_1.15_10_B_2100_mixed   1.150005  1.150045  1     2000

   co_1.15_12_X_1000_mixed   1.150005  1.150032  40    900

   co_1.15_15_X_1500_mixed   1.150005  1.150020  5     1400

   co_1.15_20_X_700_mixed    1.150005  1.150014  45    600