Image Details

Choose export citation format:

Exploring Warm Jupiter Migration Pathways with Eccentricities. II. Correlations with Host Star Properties and Orbital Separation

  • Authors: Marvin Morgan, Brendan P. Bowler, Quang H. Tran

Marvin Morgan et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 5.

Underlying eccentricity distribution results from our HBM for all warm Jupiters. The blue curve displays the median inferred underlying e distributions modeled by the Beta distribution. Solid lines represent a truncated Gaussian hyperprior, while the dashed lines represent a log-uniform hyperprior. Thin lines in the background show randomly sampled distributions from the α and β hyperparameter posteriors. A summation of the eccentricity posteriors is plotted as a histogram in gray.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse