# Asteroseismology of the exoplanet-host F-type star 94 Ceti : impact of atomic diffusion on the stellar parameters

## TL;DR

This study uses asteroseismology to analyze the exoplanet-host star 94 Ceti A, demonstrating how atomic diffusion with radiative accelerations affects stellar parameters and refining the star's characteristics.

## Contribution

It provides the first detailed asteroseismic analysis of 94 Ceti A, highlighting the impact of atomic diffusion on stellar parameter determination.

## Key findings

- Atomic diffusion with radiative accelerations can alter stellar age estimates by a few percent.
- Including a complete atmosphere in models has minimal impact on derived parameters.
- Precise stellar parameters for 94 Ceti A were obtained through combined observational and modeling efforts.

## Abstract

A precision of order one percent is needed on the parameters of exoplanet-hosts stars in order to correctly characterize the planets themselves. This will be achieved by asteroseismology. It is important in this context to test the influence on the derived parameters of introducing atomic diffusion with radiative accelerations in the models. In this paper, we begin this study with the case of the star 94 Ceti A. We performed a complete asteroseismic analysis of the exoplanet-host F-type star 94 Ceti A, from the first radial-velocity observations with HARPS up to the final computed best models. This star is hot enough to suffer from important effects of atomic diffusion, including radiative accelerations. We tested the influence of such effects on the computed frequencies and on the determined stellar parameters. We also tested the effect of including a complete atmosphere in the stellar models. The radial velocity observations were done with HARPS in 2007. The low degree modes were derived and identified using classical methods and compared with the results obtained from stellar models computed with the Toulouse Geneva Evolution Code (TGEC). We obtained precise parameters for the star 94 Ceti A. We showed that including atomic diffusion with radiative accelerations can modify the age by a few percents, whereas adding a complete atmosphere does not change the results by more than one percent.