2011/09/01 by S. Hekker, Hekker, S., T. Morel +9
Physics and Astronomy · #FOS: Physical sciences #Solar and Stellar Astrophysics (astro-ph.SR) #astro-ph.SR
paper · pdf · doi:10.48550/arxiv.1109.0148
2 pages, 1 table, 1 figure, proceedings for the second CoRoT symposium
arxiv created 2011/09/02 · arxiv updated 2011/09/05
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.