ATA: A computer code for calculation of model stellar atmospheres

version 028

The computer code ATA solves the model stellar atmosphere (generally NLTE) for given effective temperature, log g (gravitational acceleration at the stellar surface), and stellar radius. The atmosphere is represented with ND depth points.

Basic methods used in the code:

Basic options:

Input files

Output files


Program is available upon request.

Jiří Kubát
Astronomical Institute
251 65 Ondřejov
Czech Republic

Last update: 19.1.2006