Solar-Like Oscillations of Procyon A: Stellar Models and Time Series Simulations versus Observations
Abstract
The aim of this paper (further developed in Barban et al. 1999) is to present new evidence of the possible stellar origin of the observed excess power in the power spectrum of Procyon A presented in Martic et al. (1999) by comparing these observational data with theoretical predictions and numerical simulations.
- Publication:
-
IAU Colloq. 176: The Impact of Large-Scale Surveys on Pulsating Star Research
- Pub Date:
- 2000
- Bibcode:
- 2000ASPC..203..461B