Interrelated main-sequence MLR, MRR, MTR relations from planet hosting stars

Bakış V., Eker Z., Soydugan F., Bilir S.

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.