Interrelated main-sequence MLR, MRR, MTR relations from planet hosting stars
Binary and Multiple Stars in the Era of Big Sky Surveys, Brno, Çek Cumhuriyeti, 9 - 13 Eylül 2024, cilt.55, sa.3, ss.234-237, (Tam Metin Bildiri)
- Yayın Türü: Bildiri / Tam Metin Bildiri
- Cilt numarası: 55
- Doi Numarası: 10.31577/caosp.2025.55.3.234
- Basıldığı Şehir: Brno
- Basıldığı Ülke: Çek Cumhuriyeti
- Sayfa Sayıları: ss.234-237
- İstanbul 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.