Below, we present links to a complete bank of g-mode adiabatic pulsation periods appropriate for asteroseismology of ZZ Ceti stars. These periods were computed on state-of-the-art DA white dwarf models generated taking into account the complete evolutionary history of the progenitor stars. These models are characterized by self-consistent chemical profiles from the centre to the surface, and as such, they are particularly suitable to perform asteroseismological studies. We also provide chemical profiles and the run of the Brunt-Väisälä and Lamb frequencies for our complete set of DA white dwarf models. The computations cover a range of effective temperature (15,000 – 10,000 K) that amply embraces the observed ZZ Ceti instability strip.
The results presented below have been published in the following papers:
New chemical profiles for the asteroseismology of ZZ Ceti stars, Althaus, L. G.; Córsico, A. H., Bischoff-Kim, A., Romero, A. D., Renedo, I., García-Berro, E., Miller Bertolami, M. M. 2010, ApJ, 717, 897
Toward ensemble asteroseismology of ZZ Ceti stars with fully evolutionary models, Romero, A. D., Córsico, A. H., Althaus, L. G., Kepler, S. O., Castanheira, B. G., & Miller Bertolami, M. M. 2012, MNRAS, 420, 1462
Astrosismología de estrellas ZZ Ceti, Romero, A. D. 2012, PhD Thesis, Universidad de Buenos Aires
The data are organized in three tables: