Slow strangulation quenching, acting over long star formation timescales in low-mass galaxies, explains why passive galaxies have higher stellar metallicities than star-forming galaxies of the same mass.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
The origin of the metallicity difference between star-forming and passive galaxies: Insights from {\nu}2GC semi-analytic model
Slow strangulation quenching, acting over long star formation timescales in low-mass galaxies, explains why passive galaxies have higher stellar metallicities than star-forming galaxies of the same mass.