Investigation of three red giants observed in the CoRoT seismo field
S. Hekker, T. Morel, A. Mazumdar, F. Baudin, E. Poretti, M.Rainer
TL;DR
This study analyzes three red giants observed in the CoRoT field, combining space-based and ground-based data with stellar models to understand their properties.
Contribution
It provides a detailed analysis of three red giants using combined observational data and stellar evolution modeling, which is a novel integrated approach.
Findings
Preliminary stellar parameters derived from combined data.
Insights into the internal structure of the red giants.
Enhanced understanding of red giant evolution.
Abstract
Three red giants (HD 49566 (G5III), HD 169370 (K0III) and HD 169751 (K2III)) have been observed in the CoRoT seismo field and additional ground-based spectra have been acquired. We present preliminary results of a detailed study of these stars using the observational constraints from the spectra and CoRoT data, and models from the YREC stellar evolution code.
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Astronomical Observations and Instrumentation