Asteroseismic modelling of Procyon A: Preliminary results

TL;DR

This paper reports preliminary asteroseismic modeling of Procyon A, comparing model-predicted frequencies with observed data under two mode identification scenarios to improve understanding of the star's internal structure.

Contribution

It introduces a new preliminary modeling approach for Procyon A, incorporating two different mode identification scenarios based on recent observations.

Findings

Model frequencies compared with observed data

Two mode identification scenarios tested

Initial insights into Procyon A's internal structure

Abstract

We present our preliminary results of the modelling of the F5 star Procyon A. The frequencies predicted by our models are compared with the frequencies extracted through a global fit to the power spectrum obtained by the latest ground-based observations, which provides two different mode identification scenarios.