Nesibe ÖZEL

7285

Differential Seismic Modelling of Solar-like Stars

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”.
Keywords:

stars: pulsating, stars: oscillations exoplanets,

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  • Nesibe Özel, 19. Ulusal Astronomi Kongresi: UAK 2015, 2 - 6 Şubat 2015, Ankara, Orta Doğu Teknik Üniversitesi.
Turkish Journal of Astronomy and Astrophysics-Cover
  • Yayın Aralığı: Yılda 2 Sayı
  • Başlangıç: 2020
  • Yayıncı: Türk Astronomi Derneği
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