Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT 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 3.

Plotted in orange is the metallicity distribution of ≈20,000 field stars in the solar neighborhood within ∼40 pc (B. Nordström et al. 2004). The blue histogram shows the metallicity distribution of warm Jupiter host stars in this study. These hosts are, on average, more metal-rich than the field star population.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse