Interrelated main-sequence MLR, MRR, MTR relations from planet hosting stars
Contributions of the Astronomical Observatory Skalnate Pleso, vol.55, no.3, pp.234-237, 2025 (SCI-Expanded)
- Publication Type: Article / Article
- Volume: 55 Issue: 3
- Publication Date: 2025
- Doi Number: 10.31577/caosp.2025.55.3.234
- Journal Name: Contributions of the Astronomical Observatory Skalnate Pleso
- Journal Indexes: Science Citation Index Expanded (SCI-EXPANDED), Scopus
- Page Numbers: pp.234-237
- Keywords: stars:fundamental parameters, stars:host stars
- Akdeniz University Affiliated: Yes
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.