Different quenching tracers applied to MaNGA galaxies produce varying inside-out versus outside-in fractions, with inside-out rising at higher stellar mass while halo-mass trends are weaker.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Inside-Out vs. Outside-In Quenching of MaNGA Galaxies: Dependence on Stellar Mass and Environment
Different quenching tracers applied to MaNGA galaxies produce varying inside-out versus outside-in fractions, with inside-out rising at higher stellar mass while halo-mass trends are weaker.