Conference Paper

Differential Seismic Modelling of Solar-like Stars

Volume: 1 Number: 1 December 11, 2020
  • Nesibe Özel *
EN

Differential Seismic Modelling of Solar-like Stars

Abstract

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

References

  1. Nesibe Özel, 19. Ulusal Astronomi Kongresi: UAK 2015, 2 - 6 Şubat 2015, Ankara, Orta Doğu Teknik Üniversitesi.

Details

Primary Language

English

Subjects

Astronomical Sciences (Other)

Journal Section

Conference Paper

Authors

Nesibe Özel * This is me
Türkiye

Publication Date

December 11, 2020

Submission Date

September 18, 2015

Acceptance Date

-

Published in Issue

Year 2020 Volume: 1 Number: 1

TJAA is a publication of Turkish Astronomical Society (TAD).