γ Bootis: Asteroseismology with a 1-m Class Telescope
Abstract
High-resolution spectroscopic observations carried out in 2005, allowed Ventura et al. (2007) to identify oscillation modes on the rapidly rotating δ Scuti star γ Bootis. Here we consider the theoretical interpretation of the observed oscillation spectrum based on structure models and oscillation frequencies calculated by including effects due to the fast rotation.
- Publication:
-
Unsolved Problems in Stellar Physics: A Conference in Honor of Douglas Gough
- Pub Date:
- November 2007
- DOI:
- 10.1063/1.2819010
- Bibcode:
- 2007AIPC..948..455D
- Keywords:
-
- 95.55.-n;
- 97.10.Sj;
- 97.10.Kc;
- 96.60.Ly;
- Astronomical and space-research instrumentation;
- Pulsations oscillations and stellar seismology;
- Stellar rotation;
- Helioseismology pulsations and shock waves