The directories contain stellar models made with the Eggleton
code as described in

"Stellar evolution models for Z = 0.0001 to 0.03"

Pols, Onno R., Schroder, Klaus-Peter, Hurley, Jarrod R., Tout,
Christopher A. and Eggleton, Peter P.

1998 MNRAS 298, 525

All are gzipped.  Files ending .out are detailed model output while
files ending .mod are the input files for the code.

As an example

m00110z0003ov12.out

contains output for a star of mass 1.1Msun, metallicity Z = 0.0003 and
convective overshooting parameter 0.12.

Where a helium flash takes place at low masses the evolution is
continued in files of the same name but with the initial 'm' replaced
by a 'p'.

Internal output is given every 300 models and is largely self
explanatory.

The short summary can be deciphered using the following key:

*  1 Mstar   2 dty     3 tn      4 per     5 LH      6 Lth     7 CXH     8 CXHe
*  9 CXC    10 CXN    11 CXO    12 CXNe   13 CXMg   14 Cpsi   15 Crho   16 CT
* 17 MHcr   18 age    19 tKH    20 RLF    21 LHe    22 Lneu   23 SXH    24 SXHe
* 25 SXC    26 SXN    27 SXO    28 SXNe   29 SXMg   30 Spsi   31 Srho   32 ST
* 33 MHecr  34 MHtot  35 MHetot 36 Mbin   37 Mdot   38 LCO    39 MTmax  40 TmXH
* 41 TmXHe  42 TmXC   43 TmXN   44 TmXO   45 TmXNe  46 TmXMg  47 Tmpsi  48 Tmrho
* 49 Tmax   50 MCcr   51 conv1  52 conv2  53 conv3  54 conv4  55 conv5  56 conv6
* 57 conv7  58 conv8  59 conv9  60 conv10 61 conv11 62 conv12 63 Ienv   64 k**2 
* 65 per0   66 Srad   67 Slum

where S refers to the surface, C to the centre and Tm to the
temperature maximum within the star.