Constraining planet structure and composition from stellar chemistry: trends in different stellar populations

2017/11/02 by N. C. Santos, V. Adibekyan, Caroline Dorn +12 · 2 citations
Physics and Astronomy · #Astro and Planetary Science #Astrobiology #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Exoplanet #Physics #Planet #Stars #Stellar atmosphere #Stellar collision #Stellar evolution #Stellar structure #Stellar, planetary, and galactic studies #astro-ph.EP

paper · pdf · doi:10.1051/0004-6361/201731359

published as A&A 608, A94 (2017) · Accepted for publication in Astronomy & Astrophysics

arxiv created 2017/11/02 · openalex publication_date 2017/12/01 · arxiv updated 2017/12/13 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06

Abstract

Context. The chemical composition of stars that have orbiting planets provides important clues about the frequency, architecture, and composition of exoplanet systems.

Citations

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Cited by

• Masses for the seven planets in K2-32 and K2-233
• The Chemical Homogeneity of Sun-like Stars in the Solar Neighborhood