4 citations · 7 across the 6 of their papers we have counts for
7 papers
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…
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…
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…
The Role of Asteroseismology in Understanding Mass Loss in Red Giants
Sibel Örtel, Mutlu Yıldız
Red giant stars play a key role in advancing our understanding of stellar mass loss. However, its initial mass and the amount of mass lost during this phase remain uncertain. In th…
Is there a unique asteroseismic interior model for the solar-like oscillating KIC 7747078?
Sibel Örtel, Mutlu Yıldız, Z. Çelik
Asteroseismology provides a direct observational window into the structure and evolution of stars. While spectroscopic and photometric methods only provide information about the su…
The Gasing Pangkah Collaboration: I. Asteroseismic Identification and Characterisation of a Rapidly-Rotating Engulfment Candidate
J. M. Joel Ong, Marc Teng Yen Hon, Melinda Soares-Furtado +19
We report the discovery and characterisation of TIC 350842552 ("Zvrk"), an apparently isolated, rapidly-rotating () red giant observed by TESS in…
TESS Asteroseismology of Mensae: Benchmark Ages for a G7 Dwarf and its M-dwarf Companion
Ashley Chontos, Daniel Huber, Travis A. Berger +27
Asteroseismology of bright stars has become increasingly important as a method to determine fundamental properties (in particular ages) of stars. The Kepler Space Telescope initiat…