Homogeneous SpeX metallicities of M-dwarf planet hosts show sub-Neptune hosts are more metal-rich than super-Earth hosts, supporting ice-line formation plus migration.
Title resolution pending
1 Pith paper cite this work, alongside 96 external citations. Polarity classification is still indexing.
1
Pith paper citing it
96
external citations · OpenAlex
fields
astro-ph.EP 1years
2026 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Uniform Metallicity Measurements of M Dwarf Planet Hosts Support Metallicity-Dependent Sub-Neptune Formation
Homogeneous SpeX metallicities of M-dwarf planet hosts show sub-Neptune hosts are more metal-rich than super-Earth hosts, supporting ice-line formation plus migration.