Published January 1, 2025
| Version v1
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Interrelated main-sequence MLR, MRR, MTR relations from planet hosting stars
Creators
- 1. Akdeniz Univ, Fac Sci, Dept Space Sci & Technol, Antalya, Turkiye
- 2. Canakkale Onsekiz Mart Univ, Fac Sci, Dept Phys, Canakkale, Turkiye
- 3. Istanbul Univ, Fac Sci, Dept Astron & Space Sci, Istanbul, Turkiye
Description
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.
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