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ZENODO
Presentation . 2021
License: CC BY
Data sources: Datacite
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ZENODO
Presentation . 2021
License: CC BY
Data sources: Datacite
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Other literature type . 2021
License: CC BY
Data sources: ZENODO
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Star Formation and Quenching in High-redshift Clusters: A view of gas, mass, and stars

descriptionPublicationkeyboard_double_arrow_right Presentation , Other literature type 23 Jun 2021Publisher:Zenodo
Authors: Allison G Noble;

doi: 10.5281/zenodo.5016146 , 10.5281/zenodo.5016147

Star Formation and Quenching in High-redshift Clusters: A view of gas, mass, and stars

Abstract

The effect of the cluster environment on the star formation and quenching of high redshift galaxies has been elusive. However, technological capabilities and dedicated spectroscopic campaigns have opened a new window onto these processes within massive, virialized clusters at z~1 and all the way back to filamentary, extended protoclusters at z>2. I will review progress we have made on these fronts through the lens of gas, mass, and stars within high-redshift (proto)cluster galaxies, focusing in particular on recent clues into environmental quenching from ALMA.

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This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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