Radiative acceleration calculation methods and abundance anomalies in Am stars

This archive contains stellar structures used to create the figures of surface abundance evolution with time of the paper entitled "Radiative acceleration calculation methods and abundance anomalies in Am stars" to be published in Astronomy & Astrophysics.

The first directory level refers to the dataset used to compute the Rosseland mean opacities (OP = Opacity Project for instance), the second to the stellar mass (in solar mass unit), and the third to the g_rad calculation method and the prescriptions used for macroscopic transport processes (e.g. SVP2004_RMT for g_rad computed with the 2004 version of the SVP approximation and the RMT turbulence model).

In each of these directories, the stellar structure file name contains the age (e.g. "structure.00215.78.gz" for an age of 215.78 Myr). 

The first line of each stellar structure file shows the meaning of each field. The columns are separated with tabulations to allow easy an importation in spreadsheets. All quantities are expressed in cgs units, the abundances in mass fractions.