CAOSP abstracts, Volume: 55, No.: 3, year: 2025

Author(s): Bakış, V.; Eker, Z.; Soydugan, F.; Bilir, S.
Journal: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 55, no. 3, p. 234-237.
Date: 04/2025
Title: Interrelated main-sequence MLR, MRR, MTR relations from planet hosting stars
Keyword(s): stars:fundamental parameters, stars:host stars
Pages: 234 -- 237
DOI: https://doi.org/10.31577/caosp.2025.55.3.234
NASA ADS Abstract Service: 2025CoSka..55c.234B
Citation:
License: This work is licensed under a Creative Commons Attribution 4.0 International License

Abstract: In this study, we investigated the interrelated mass-luminosity, mass-radius, and mass-temperature relations of planet-hosting stars. The sample, which is chosen to be main-sequence systems, is divided into two metallicity regimes: one regime is below the average of all samples (z=0.017) and the other above it. Suitable figures represent the comparisons of each distinct metallicity regime.