Reference grids of stellar models and oscillation frequencies: Data from the CESAM stellar evolution code and ADIPLS oscillation programme
arXiv:0808.4105 · doi:10.1007/s10509-008-9781-z
Abstract
We present grids of stellar models and their associated oscillation frequencies that have been used by the CoRoT Seismology Working Group during the scientific preparation of the CoRoT mission. The stellar models have been calculated with the CESAM stellar internal structure and evolution code while the oscillation frequencies have been obtained from the CESAM models by means of the ADIPLS adiabatic oscillation programme. The grids cover a range of masses, chemical compositions and evolutionary stages corresponding to those of the CoRoT primary targets. The stellar models and oscillation frequencies are available on line through the Evolution and Seismic Tools Activity (ESTA) web site.
5 pages, 3 figures accepted for publication in ApSS (CoRoT/ESTA special volume)
References in corpus (10)
- ADIPLS -- the Aarhus adiabatic oscillation package
- A Realistic Determination of the Error on the Primordial Helium Abundance: Steps Toward Non-Parametric Nebular Helium Abundances
- CESAM: a free code for stellar evolution calculations
- CoRoT/ESTA-TASK 1 and TASK 3 comparison of the internal structure and seismic properties of representative stellar models: Comparisons between the ASTEC, CESAM, CLES, GARSTEC and STAROX codes
- The CoRoT Evolution and Seismic Tools Activity: Goals and Tasks
- Inter-comparison of the g-, f- and p-modes calculated using different oscillation codes for a given stellar model
- Grids of stellar evolution models for asteroseismology (CESAM + POSC)
- Preparing the COROT space mission: new variable stars in the galactic Anticenter direction
- Thorough analysis of input physics in CESAM and CLES codes
- Grids of Stellar Models and Frequencies with CLES + LOSC