# Compact star-forming galaxies preferentially quenched to become PSBs in z < 1 clusters

@article{Socolovsky2019CompactSG,
title={Compact star-forming galaxies preferentially quenched to become PSBs in z < 1 clusters},
author={M. Socolovsky and D. Maltby and N. Hatch and O. Almaini and V. Wild and W. Hartley and C. Simpson and Kate Rowlands Nottingham and S. Andrews and Ucl and G. Observatory and Johns Hopkins},
journal={Monthly Notices of the Royal Astronomical Society},
year={2019},
volume={482},
pages={1640-1650}
}
MS acknowledges support from IAC and STFC. VW acknowledges support from the European Research Council Starting grant (SEDmorph, P.I. V. Wild).

#### Paper Mentions

HST/WFC3 grism observations of z ∼ 1 clusters: evidence for evolution in the mass–size relation of quiescent galaxies from post-starburst galaxies
• J Matharu, A Muzzin, +10 authors G Wilson
• Physics
• 2020
Minor mergers have been proposed as the driving mechanism for the size growth of quiescent galaxies with decreasing redshift. The process whereby large star-forming galaxies quench and join theExpand
Extended star-forming region within galaxies in a dense proto-cluster core at z=2.53.
At $z\sim2$, star-formation activity is thought to be high even in high-density environments such as galaxy clusters and proto-clusters. One of the critical but outstanding issues is if structuralExpand
Implications of Increased Central Mass Surface Densities for the Quenching of Low-mass Galaxies
We use the Cosmic Assembly Deep Near-infrared Extragalactic Legacy Survey data to study the relationship between quenching and the stellar mass surface density within the central radius of 1 kpc (Σ1)Expand
Mergers, Starbursts, and Quenching in the Simba Simulation.
• Physics
• 2019
We use the Simba cosmological galaxy formation simulation to investigate the relationship between major mergers ($\leq$ 4:1), starbursts, and galaxy quenching. Mergers are identified via sudden jumpsExpand
Molecular gas in distant brightest cluster galaxies
• Physics
• 2019
The stellar mass assembly of brightest cluster galaxies (BCGs) is still debated. We have observed in CO with the IRAM-30m two star forming BCGs belonging to SpARCS clusters, 3C 244.1 ($z=0.4$) andExpand
The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations.
• Physics
• 2019
As demonstrated in Paper I, the quenching properties of central and satellite galaxies are quite similar as long as both stellar mass and halo mass are controlled. Here we extend the analysis to theExpand
The Morphology–Density Relationship in 1 < z < 2 Clusters
The morphology-density relationship states that dense cosmic environments such as galaxy clusters have an overabundance of quiescent elliptical galaxies, but it is unclear at which redshift thisExpand

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