Yayınlanmış 1 Ocak 2025
| Sürüm v1
Dergi makalesi
Açık
Interrelated main-sequence MLR, MRR, MTR relations from planet hosting stars
Oluşturanlar
- 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
Açıklama
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.
Dosyalar
bib-3fe25ed6-94b0-4279-954c-fab53c8f25f4.txt
Dosyalar
(209 Bytes)
| Ad | Boyut | Hepisini indir |
|---|---|---|
|
md5:c0a5824e77e55d972b24a0724a3feda3
|
209 Bytes | Ön İzleme İndir |