Fast-rotating green valley galaxies maintain higher metallicities than slow-rotating ones because slow rotators experience stronger outflows and more mergers that deplete their chemical content.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
years
2026 3verdicts
UNVERDICTED 3representative citing papers
An analytical model of galaxies evolving along the star-forming main sequence shows that episodic quiescence or late assembly is required to reproduce observed star formation histories and avoid over-massive galaxies today.
The paper proposes the SHARP near-IR spectrograph design for ESO's ELT, split into NEXUS MOS and VESPER multi-IFU units, to address questions from primordial galaxies to nearby star formation.
citing papers explorer
-
Contrasting evolutionary pathways of fast- and slow-rotating galaxies in the green valley
Fast-rotating green valley galaxies maintain higher metallicities than slow-rotating ones because slow rotators experience stronger outflows and more mergers that deplete their chemical content.
-
Built to Rest: The Evolving Star-Forming Main Sequence Requires Episodic Quiescence or Late Assembly
An analytical model of galaxies evolving along the star-forming main sequence shows that episodic quiescence or late assembly is required to reproduce observed star formation histories and avoid over-massive galaxies today.
-
SHARP -- A spectrograph proposal to fully exploit ELT capabilities and look beyond JWST
The paper proposes the SHARP near-IR spectrograph design for ESO's ELT, split into NEXUS MOS and VESPER multi-IFU units, to address questions from primordial galaxies to nearby star formation.