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Spectrum Analysis of Bright Kepler Gamma Doradus Candidate Stars

Tkachenko, Andrew; Lehmann, Holger; Smalley, Barry; Debosscher, Jonas; Aerts, Conny

Authors

Andrew Tkachenko

Holger Lehmann

Jonas Debosscher

Conny Aerts



Abstract

Ground-based spectroscopic follow-up observations of the pulsating stars observed by the Kepler satellite mission are needed for their asteroseismic modelling. We aim to derive the fundamental parameters for a sample of 26 Gamma Doradus candidate stars observed by the Kepler satellite mission to accomplish one of the required preconditions for their asteroseismic modelling and to compare our results with the types of pulsators expected from the existing light curve analysis. We use the spectrum synthesis method to derive the fundamental parameters like Teff, logg, [M/H], and vsini from newly obtained spectra and compute the spectral energy distribution from literature photometry to get an independent measure of Teff. We find that most of the derived Teff values agree with the values given in the Kepler Input Catalogue. According to their positions in the HR-diagram three stars are expected Gamma Dor stars, ten stars are expected Delta Sct stars, and seven stars are possibly Delta Sct stars at the hot border of the instability strip. Four stars in our sample are found to be spectroscopic binary candidates and four stars have very low metallicity where two show about solar C abundance. Six of the 10 stars located in the Delta Sct instability region of the HR-diagram show both Delta Sct and Gamma Dor-type oscillations in their light curves implying that Gamma Dor-like oscillations are much more common among the Delta Sct stars than predicted by theory. Moreover, seven stars showing periods in the Delta Sct and the Delta Sct-Gamma Dor range in their light curves are located in the HR-diagram left of the blue edge of the theoretical Delta Sct instability strip. The consistency of these findings with recent investigations based on high-quality Kepler data implies the need for a revision of the theoretical Gamma Dor and Delta Sct instability strips.

Citation

Tkachenko, A., Lehmann, H., Smalley, B., Debosscher, J., & Aerts, C. (2012). Spectrum Analysis of Bright Kepler Gamma Doradus Candidate Stars. Monthly Notices of the Royal Astronomical Society, 422(4), 2960–2968. https://doi.org/10.1111/j.1365-2966.2012.20687.x

Journal Article Type Article
Acceptance Date Feb 3, 2012
Online Publication Date May 21, 2012
Publication Date 2012-06
Deposit Date Jul 6, 2023
Publicly Available Date Jul 6, 2023
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 422
Issue 4
Pages 2960–2968
DOI https://doi.org/10.1111/j.1365-2966.2012.20687.x
Keywords Solar and Stellar Astrophysics