Traversing the Star-forming Main Sequence with Molecular Gas Stacks of z ∼ 1.6 Cluster Galaxies

Traversing the Star-forming Main Sequence with Molecular Gas Stacks of z ∼ 1.6 Cluster Galaxies

The cluster environment has been shown to affect the molecular gas content of cluster members, yet a complete understanding of this often subtle effect has been hindered due to a lack of detections over the full parameter space of galaxy star formation rates (SFRs) and stellar masses. Here, we stack...

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Bibliographic Details
Main Authors: Alex Pigarelli, Allison Noble, Gregory Rudnick, William Cramer, Stacey Alberts, Yannick Bahe, Patrick S. Kamieneski, Sebastian Montaño, Adam Muzzin, Julie Nantais, Sarah Saavedra, Eelco van Kampen, Tracy Webb, Christina C. Williams, Gillian Wilson, H. K. C. Yee
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Galaxy clusters
High-redshift galaxy clusters
Galactic and extragalactic astronomy
Radio astronomy
Molecular gas
Online Access:https://doi.org/10.3847/1538-4357/adc99e
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