Slow-then-rapid quenching as traced by tentative evidence for enhanced metallicities of cluster galaxies at z ~ 0.2 in the slow quenching phase

TY - JOUR

T1 - Slow-then-rapid quenching as traced by tentative evidence for enhanced metallicities of cluster galaxies at z ~ 0.2 in the slow quenching phase

AU - Maier, C.

AU - Ziegler, B. L.

AU - Haines, C. P.

AU - Smith, G. P.

N1 - Publisher Copyright: © ESO 2019.

PY - 2019/1

Y1 - 2019/1

KW - galaxies: evolution

KW - galaxies: clusters: general

KW - galaxies: star formation

KW - galaxies: abundances

KW - ASSEMBLY HISTORY

KW - CLASSIFICATION

KW - LUMINOSITY FUNCTION

KW - ORIGIN

KW - EVOLUTION

KW - STAR-FORMATION RATES

KW - GAS

KW - SIMULATIONS

KW - STELLAR MASS

KW - SUBSTRUCTURE

KW - Galaxies: Abundances

KW - Galaxies: Clusters: General

KW - Galaxies: Evolution

KW - Galaxies: Star formation

UR - http://www.scopus.com/inward/record.url?scp=85060399834&partnerID=8YFLogxK

U2 - 10.1051/0004-6361/201834290

DO - 10.1051/0004-6361/201834290

M3 - Article

SN - 0004-6361

VL - 621

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

M1 - A131

ER -