The files iRAWD_feh*_elements.txt and iRAWD_feh*_isotopes.txt contain
the lists of elemental and isotopic abundances (mass fractions) at
the surfaces of the He convective zones in our RAWD models
at the end of H ingestion. * in the names of these files indicates
the assumed [Fe/H] ratio, e.g. m2.6 means [Fe/H]=-2.6 (m stands
for the minus sign).

This directory also contains the files with the corresponding
initial abundances, e.g. iniab3.2E-04As09_fehm2.3.ppn is a list of
the initial abundances of stable isotopes for the iRAWD model
with [Fe/H]=-2.3.

The file iniab1.4E-02As09_feh0.0.ppn actually provides the solar system
abundances from Asplund et al. (2009) that were used to prepare
the initial abundances for our RAWD models.

All the RAWD models have masses close to 0.73 Msun.