Star formation and quenching among the most massive galaxies at z ∼ 1.7
about
The Evolution of Gas Content and Star Formation from z=3 to z=0Observational evidence of a slow downfall of star formation efficiency in massive galaxies during the past 10 GyrActive galactic nuclei from He ii: a more complete census of AGN in SDSS galaxies yields a new population of low-luminosity AGN in highly star-forming galaxies
P2860
Star formation and quenching among the most massive galaxies at z ∼ 1.7
description
im April 2015 veröffentlichter wissenschaftlicher Artikel
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wetenschappelijk artikel
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наукова стаття, опублікована у квітні 2015
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name
Star formation and quenching among the most massive galaxies at z ∼ 1.7
@en
Star formation and quenching among the most massive galaxies at z ∼ 1.7
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type
label
Star formation and quenching among the most massive galaxies at z ∼ 1.7
@en
Star formation and quenching among the most massive galaxies at z ∼ 1.7
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prefLabel
Star formation and quenching among the most massive galaxies at z ∼ 1.7
@en
Star formation and quenching among the most massive galaxies at z ∼ 1.7
@nl
P2093
P2860
P50
P356
P1476
Star formation and quenching among the most massive galaxies at z ∼ 1.7
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P2093
P2860
P304
P356
10.1093/MNRAS/STV608
P407
P577
2015-04-20T00:00:00Z
P818
1503.06107
P819
2015MNRAS.450..763M