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

  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},
MS acknowledges support from IAC and STFC. VW acknowledges support from the European Research Council Starting grant (SEDmorph, P.I. V. Wild). 
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
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Funding: MS acknowledges support from IAC and STFC. VW acknowledges support from the European Research Council Starting grant (SEDmorph, P.I. V. Wild).
The structure of post-starburst galaxies at 0.5 < z < 2 : evidence for two distinct quenching routes at different epochs
Funding: DTM acknowledges support from STFC. NAH acknowledges support from STFC throughan Ernest Rutherford Fellowship.
The origins of post-starburst galaxies at z <0.05
MMP, VW, JM-A, NJ and KR acknowledge support of the European Research Council via the award of a starting grant (SEDMorph; P.I. V. Wild). LTA acknowledges support from the Iraqi Ministry of HigherExpand
Star Formation in Cluster Galaxies at 0.2
The rest-frame equivalent width of the [OII] λ3727 emission line, W0(O II), has been measured for cluster and field galaxies in the Canadian Network for Observational Cosmology redshift survey ofExpand
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Galactic winds are a prime suspect for the metal enrichment of the intergalactic medium (IGM) and may have a strong influence on the chemical evolution of galaxies and the nature of QSOExpand
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