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astro-ph.SR2026
New scaling relations from MESA models for mass and radius of subgiant stars: application to Kepler targets
T. Çakır Alsaç, M. Yıldız, S. Örtel
The precise determination of the fundamental parameters of stars is crucial for understanding stellar structure and evolution. In this regard, the asteroseismic parameters of solar…
astro-ph.SR2026★ 1 cited
Asteroseismic analysis of red giants in eclipsing binaries using two methods: implications for scaling relations and chemical composition
M. Yıldız, S. Örtel, T. Çakır Alsaç
The study of solar-like oscillating red giants in eclipsing binaries (EBs) provides a unique opportunity to advance stellar astrophysics by combining dynamical mass and radius meas…
astro-ph.SR2026
Planetary systems in the light of asteroseismology: metallicity threshold for the planetary systems and age-metallicity relation
M. Yıldız, A. Demirkol, S. Örtel +2
We compiled data for 127 hosts (plus six candidates) and used them as constraints to construct interior models of the hosts using the {\small MESA} code. Two significant conclusion…