CoRoT (Convection Rotation and planetary Transits) observations provide the opportunity to study a large sample of stars ranging from the Main Sequence (MS) to the Red Giant Branch. With the large increase in the number of stars showing solar-like oscillations, we intend to extract as much information as possible from a low signal-to-noise ratio (SNR) oscillation spectrum, benefiting from comparison with a reference star having similar seismic and fundamental parameters. We propose a differential method to determine stellar properties of solar-like oscillations which we call “differential seismology of stellar twins”.
Primary Language | English |
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Subjects | Astronomical Sciences (Other) |
Journal Section | Conference Paper |
Authors | |
Publication Date | December 11, 2020 |
Submission Date | September 18, 2015 |
Published in Issue | Year 2020 Volume: 1 Issue: 1 |
TJAA is a publication of Turkish Astronomical Society (TAD).