Quenching of star formation from a lack of inflowing gas to galaxies-Reference-Cited by-同舟云学术

Quenching of star formation from a lack of inflowing gas to galaxies

Published:2021-09-22 Issue:7877 Volume:597 Page:485-488
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Whitaker Katherine E.^ORCID,Williams Christina C.^ORCID,Mowla Lamiya^ORCID,Spilker Justin S.,Toft Sune^ORCID,Narayanan Desika,Pope Alexandra^ORCID,Magdis Georgios E.^ORCID,van Dokkum Pieter G.,Akhshik Mohammad,Bezanson Rachel^ORCID,Brammer Gabriel B.^ORCID,Leja Joel^ORCID,Man Allison^ORCID,Nelson Erica J.,Richard Johan,Pacifici Camilla,Sharon Keren^ORCID,Valentino Francesco

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

https://www.nature.com/articles/s41586-021-03806-7.pdf

Reference63 articles.

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2. Sargent, M. et al. A direct constraint on the gas content of a massive, passively evolving elliptical galaxy at z = 1.43. Astrophys. J. 806, 20 (2015).

3. Spilker, J. et al. Molecular gas contents and scaling relations for massive, passive galaxies at intermediate redshifts from the LEGA-C survey. Astrophys. J. 860, 103 (2018).

4. Bezanson, R. et al. Extremely low molecular gas content in a compact, quiescent galaxy at z = 1.522. Astrophys. J. 873, 19 (2019).

5. Zavala, J. et al. On the gas content, star formation efficiency, and environmental quenching of massive galaxies in protoclusters at z ~ 2.0-2.5. Astrophys. J. 887, 183 (2019).

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