There are 420 models, with 42 radial distributions of mass
and 10 differente efficiencies to form stars, simulating 10
morphological types, from T=1 to 10.
Each files set give the time evolution of all important quantities for
spiral galaxies.
For each model, the following files there exist, with the information in
columns:
param it is the file input, where the initial radial distributions and
the parameters used by the model are given
msf : time, radius, mass in the halo, mass in the disk, the sfr of the
halo and sfr of the disk
disk: radius, mass of diffuse gas, molecular gas, massive stars, low.mass
stars, and remnnants in the disk
halo: radius, mass of diffuse gas, molecular gas, massive stars, low.mass
stars, and remnnants in the halo
rasne: radius supernova II in the halo, supernova II and Ia in the
disk, last columns 0,nothing
cstars: the stellar mas created in each time step
dihc: radius, abundances by mass of H, D,He3,He and C
dione: radius, abundances by mass of O,N,C13,neutron-rich elements,Ne
dimgfe: radius, abundances by mass of Mg, Si,S,Ca Fe
the same three for the halo abundances
hahc: radius, abundances by mass of H, D,He3,He and C
haone: radius, abundances by mass of O,N,C13,neutron-rich elements,Ne
hamgfe: radius, abundances by mass of Mg, Si,S,Ca Fe
All masses of disk and halo are in 10^9 units.
The abundances are in mass
The time step is 0.5 from 0 to 13 Gyr.
The SFR is in units of 19^9Msun/10^7yr and it was multiplied by a factor of 1000,
that it if you divide by 10 is in Msun/yr units
Here's a linecount of the ascii files describing on particular model