University of Hertfordshire

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From the same journal

By the same authors

The New Galaxy Evolution Paradigm Revealed by the Herschel Surveys

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Documents

  • Stephen A. Eales
  • Nathan Bourne
  • Jon Loveday
  • Kate Rowlands
  • Paul van der Werf
  • Simon Driver
  • Loretta Dunne
  • Simon Dye
  • Christina Furlanetto
  • R. J. Ivison
  • Steve J. Maddox
  • Aaron S. G. Robotham
  • Matthew W.L. Smith
  • Edward N. Taylor
  • Elisabetta Valiante
  • Angus Wright
  • Philip Cigan
  • Gianfranco de Zotti
  • Matt J. Jarvis
  • Lucia Marchetti
  • Michal J. Michalowski
  • Steve Phillipps
  • Sebastian Viaene
  • Catherine Vlahakis
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Original languageEnglish
Article numberstx2548
Pages (from-to)3507–3524
Number of pages18
JournalMonthly Notices of the Royal Astronomical Society
Volume473
Issue3
Early online date12 Oct 2017
DOIs
Publication statusPublished - 21 Jan 2018

Abstract

The Herschel Space Observatory has revealed a very different galaxyscape from that shown by optical surveys which presents a challenge for galaxy-evolution models. The Herschel surveys reveal (1) that there was rapid galaxy evolution in the very recent past and (2) that galaxies lie on a single Galaxy Sequence (GS) rather than a star-forming 'main sequence' and a separate region of 'passive' or 'red-and-dead' galaxies. The form of the GS is now clearer because far-infrared surveys such as the Herschel ATLAS pick up a population of optically red starforming galaxies that would have been classified as passive using most optical criteria. The space-density of this population is at least as high as the traditional star-forming population. By stacking spectra of H-ATLAS galaxies over the redshift range 0.001 < z < 0.4, we show that the galaxies responsible for the rapid low-redshift evolution have high stellar masses, high star-formation rates but, even several billion years in the past, old stellar populations - they are thus likely to be relatively recent ancestors of early-type galaxies in the Universe today. The form of the GS is inconsistent with rapid quenching models and neither the analytic bathtub model nor the hydrodynamical EAGLE simulation can reproduce the rapid cosmic evolution. We propose a new gentler model of galaxy evolution that can explain the new Herschel results and other key properties of the galaxy population.

Notes

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. ©: 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.

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