No CrossRef data available.
Article contents
Solar-Like Oscillations of Procyon A: Stellar Models and Time Series Simulations versus Observations1
Published online by Cambridge University Press: 12 April 2016
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.
- Type
- Part 6. Variables Close to the Main Sequence
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2000
Footnotes
Based on observations collected at the Observatoire de Haute-Provence (CNRS, France)