Seismic investigation of the {\gamma} Dor star KIC 6462033: The first results of Kepler and ground-based follow up observations

TL;DR

This study presents preliminary analysis of ground-based and Kepler data on the {b} Dor star KIC 6462033, aiming to understand its pulsational behavior and contribute to asteroseismic research.

Contribution

First combined ground-based and Kepler observations of KIC 6462033, providing initial insights into its pulsational characteristics for {b} Dor stars.

Findings

Initial detection of pulsational behavior in KIC 6462033

Identification of g-mode pulsations in the star

Foundation for detailed asteroseismic modeling

Abstract

We present the first preliminary results on the analysis of ground-based time series of the {\gamma} Dor star KIC 6462033 (TYC 3144-646-1, V = 10.83, P = 0.69686 d) as well as Kepler photometry in order to study pulsational behaviour in this star.{\gamma} Dor variables, which exhibit g-mode pulsations, are promising asteroseismic targets to understand their rich complexity of pulsational characteristics in detail. In order to achieve this goal, intensive and numerous multicolour and high resolution spectroscopic observations are also required, to complete space-based data aimed at the determination of their physical parameters.