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An ancient massive quiescent galaxy found in a gas-rich z ~ 3 group

Authors :
Kalita, Boris S.
Daddi, Emanuele
D'Eugenio, Chiara
Valentino, Francesco
Rich, R. Michael
Gómez-Guijarro, Carlos
Coogan, Rosemary T.
Delvecchio, Ivan
Elbaz, David
Neill, James D.
Puglisi, Annagrazia
Strazzullo, Veronica
Kalita, Boris S.
Daddi, Emanuele
D'Eugenio, Chiara
Valentino, Francesco
Rich, R. Michael
Gómez-Guijarro, Carlos
Coogan, Rosemary T.
Delvecchio, Ivan
Elbaz, David
Neill, James D.
Puglisi, Annagrazia
Strazzullo, Veronica
Publication Year :
2021

Abstract

Deep ALMA and HST observations reveal the presence of a quenched massive galaxy within the $z=2.91$ galaxy group RO-1001. With a mass-weighted stellar age of $1.6 \pm 0.4 \,$Gyr this galaxy is one of the oldest known at $z\sim3$, implying that most of its $10^{11}\rm \, M_{\odot}$ of stars were rapidly formed at $z>6$--8. This is a unique example of the predominantly passive evolution of a galaxy over at least $3<z<6$ following its high-redshift quenching and a smoking-gun event pointing to the early imprint of an age-environment relation. At the same time, being in a dense group environment with extensive cold-gas reservoirs as betrayed by a giant Ly$\alpha$ halo, the existence of this galaxy demonstrates that gas accretion shutdown is not necessary for quenching and its maintenance.<br />Comment: Accepted for publication in ApJL

Details

Database :
OAIster
Publication Type :
Electronic Resource
Accession number :
edsoai.on1312085945
Document Type :
Electronic Resource
Full Text :
https://doi.org/10.3847.2041-8213.ac16dc