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Asteroseismic modelling of the Binary HD 176465

B. Nsamba, M. J. P. F. G. Monteiro, T. L. Campante, D. R. Reese, T. R. White, A. GarcŪa HernŠndez, C. Jiang

Abstract
The detection and analysis of oscillations in binary star systems is critical in understanding stellar structure and evolution. This is partly because such systems have the same initial chemical composition and age. Solar-like oscillations have been detected by Kepler in both components of the asteroseismic binary HD 176465. We present an independent modelling of each star in this binary system. Stellar models generated using MESA (Modules for Experiments in Stellar Astrophysics) were fitted to both the observed individual frequencies and complementary spectroscopic parameters. The individual theoretical oscillation frequencies for the corresponding stellar models were obtained using GYRE as the pulsation code. A Bayesian approach was applied to find the probability distribution functions of the stellar parameters using AIMS (Asteroseismic Inference on a Massive Scale) as the optimisation code. The ages of HD 176465 A and HD 176465 B were found to be 2.81±0.48 Gyr and 2.52±0.80 Gyr, respectively. These results are in agreement when compared to previous studies carried out using other asteroseismic modelling techniques and gyrochronology.

Keywords
Asteroseismology - Stars; fundamental parameters - Stars; individual; HD 176465; Astrophysics - Solar and Stellar Astrophysics

Seismology of the Sun and the Distant Stars 2016 – Using Today’s Successes to Prepare the Future – TASC2 & KASC9 Workshop – SPACEINN & HELAS8 Conference
M.J.P.F.G. Monteiro, M.S. Cunha, J.M.T.S. Ferreira

EPJ Web of Conferences
Volume 160, Number 0501, Page 4
2017 October

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Instituto de Astrof√≠sica e Ci√™ncias do Espa√ßo Universidade do Porto Faculdade de Ciências da Universidade de Lisboa
Fundação para a Ciência e a Tecnologia COMPETE 2020 PORTUGAL 2020 União Europeia