Interrelated main-sequence MLR, MRR, MTR relations from planet hosting stars
Contributions of the Astronomical Observatory Skalnate Pleso, cilt.55, sa.3, ss.234-237, 2025 (SCI-Expanded)
- Yayın Türü: Makale / Tam Makale
- Cilt numarası: 55 Sayı: 3
- Basım Tarihi: 2025
- Doi Numarası: 10.31577/caosp.2025.55.3.234
- Dergi Adı: Contributions of the Astronomical Observatory Skalnate Pleso
- Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
- Sayfa Sayıları: ss.234-237
- Anahtar Kelimeler: stars:fundamental parameters, stars:host stars
- Akdeniz Üniversitesi Adresli: Evet
Özet
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.