Stellar models calculated with Cambridge STARS evolution code

Code is available from http://www.ast.cam.ac.uk/~stars/

Stellar models are used in McClelland and Eldridge (2016) and are available from http://bpass.auckland.ac.nz

Contact lmcc054@aucklanduni.ac.nz for further details.

The files are grouped as follows: plotfiles_METALLICITY_CLUMPING_MASSLOSS

MASSLOSS is the scaling factor (beta) applied to the mass-loss rate. Mass-loss scheme is taken from Nugis and Lamers (2000).

CLUMPING is the clumping factor for the inflated envelope. See Graefener et al. (2011) for details.

Each file is compressed using XZ Utils (standard on many *nix OSes, otherwise available here http://tukaani.org/xz/).

To decompress, use tar -vxJf filename.tar.xz

Columns in files are:

1) Model age in years
2) log(R/R(Sun)
3) log(T/K)
4) log(L/L(sun))
5) M(Star)/M(Sun)
6) M(Helium Core)/M(Sun)
7) M(CO core)/M(Sun)
8) Mass-loss rate (M(Sun)/yr)
9) Surface helium abundance
10) Surface Carbon abundance
11) Surface nitrogen abundance
12) Surface oxygen abundance