Giant planets around M dwarfs show lower bulk metallicities than those around FGK stars, with similar mass-metallicity slopes but a significant offset between the populations.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.EP 1years
2024 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
The bulk metallicity of giant planets around M stars
Giant planets around M dwarfs show lower bulk metallicities than those around FGK stars, with similar mass-metallicity slopes but a significant offset between the populations.