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Review of current performance of seismic diagnostics and stellar parameters determinations
Invited comunication

M. S. Cunha

Abstract

I will discuss different procedures to infer stellar fundamental parameters, namely, the stellar mass, radius, and age, from the analysis of combinations of seismic and non-seismic data. Theperformance of these procedures will be illustrated through the presentation of results obtained for simulated and space-based data. In that context, I will also briefly discuss additional seismic diagnostics that are of interest in the context of the characterization of exoplanetary systems.

The PLATO Mission Conference 2017: Exoplanetary systems in the PLATO era
Warwick, United Kingdom
2017 September

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Instituto de Astrofísica e Ciências do Espaço Universidade do Porto Faculdade de Ciências da Universidade de Lisboa
Fundação para a Ciência e a Tecnologia COMPETE 2020 PORTUGAL 2020 União Europeia