Architectures of Exoplanetary Systems. IV: A Multi-planet Model for Reproducing the Radius Valley and Intra-system Size Similarity of Planets around Kepler's FGK Dwarfs

Documenti analoghi

• The Distribution of Planet Radius in Kepler Multiplanet Systems Depends on Gap Complexity
  di: Rice, David R., et al.
  Pubblicazione: (2024)
• Exoplanet Orbital Distribution around FGK Sun-like Host Stars I: planet occurrence rate derived from the Kepler Mission and theoretical interpretations from planet formation
  di: Zeng, Li, et al.
  Pubblicazione: (2026)
• TESS Planet Occurrence Rates Reveal the Disappearance of the Radius Valley Around Mid-to-Late M Dwarfs
  di: Gillis, Erik, et al.
  Pubblicazione: (2026)
• An Oxidation Gradient Straddling the Small Planet Radius Valley
  di: Cherubim, Collin, et al.
  Pubblicazione: (2025)
• From Stability to Instability: Characterizing the Eccentricities of Multi-planet Systems in the California Kepler Survey as a Means of Studying Stability
  di: Doty, Matthew J., et al.
  Pubblicazione: (2025)