Results 131 to 140 of about 161,517 (237)

OBSERVATIONS OF ENVIRONMENTAL QUENCHING IN GROUPS IN THE 11 GYR SINCEz= 2.5: DIFFERENT QUENCHING FOR CENTRAL AND SATELLITE GALAXIES [PDF]

open access: bronze, 2014
Tomer Tal   +18 more
openalex   +1 more source

THE ISLANDS PROJECT. I. ANDROMEDA XVI, AN EXTREMELY LOW MASS GALAXY NOT QUENCHED BY REIONIZATION* [PDF]

open access: green, 2016
M. Monelli   +16 more
openalex   +1 more source

DESI Massive Poststarburst Galaxies at z ∼ 1.2 Have Compact Structures and Dense Cores

open access: yesThe Astrophysical Journal
Poststarburst galaxies (PSBs) are young quiescent galaxies that have recently experienced a rapid decrease in star formation, allowing us to probe the fast-quenching period of galaxy evolution.
Yunchong Zhang   +36 more
doaj   +1 more source

Is the cluster environment quenching the Seyfert activity in elliptical and spiral galaxies? [PDF]

open access: bronze, 2016
Rafael S. de Souza   +9 more
openalex   +1 more source

Two Distinct Classes of Quiescent Galaxies at Cosmic Noon Revealed by JWST PRIMER and UNCOVER

open access: yesThe Astrophysical Journal Letters
We present a measurement of the low-mass quiescent size–mass relation at cosmic noon (1 < z < 3) from the JWST PRIMER and UNCOVER treasury surveys, which highlights two distinct classes of quiescent galaxies.
Sam E. Cutler   +33 more
doaj   +1 more source

A massive quiescent galaxy at redshift 4.658. [PDF]

open access: yesNature, 2023
Carnall AC   +12 more
europepmc   +1 more source

The evolution of galaxies at constant number density: a less biased view of star formation, quenching, and structural formation [PDF]

open access: bronze, 2016
Jamie R. Ownsworth   +6 more
openalex   +1 more source

The cumulative star formation histories of dwarf galaxies with TNG50. I: environment-driven diversity and connection to quenching [PDF]

open access: green, 2021
Gandhali D Joshi   +7 more
openalex   +1 more source

Active Galactic Nuclei in the Green Valley at z ∼ 0.7

open access: yesThe Astrophysical Journal
We present near-infrared (NIR) spectroscopy using the MMT and Magellan infrared spectrograph for a sample of 29 massive galaxies ( $\mathrm{log}\ {M}_{* }/{M}_{\odot }\gtrsim 10$ ) at z ∼ 0.7 with optical spectroscopy from the Large Early Galaxy ...
Charity Woodrum   +7 more
doaj   +1 more source

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