The new galaxy evolution paradigm revealed by the Herschel surveys

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 si...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2018-01, Vol.473 (3), p.3507-3524
Hauptverfasser: Eales, Stephen, Smith, Dan, Bourne, Nathan, Loveday, Jon, Rowlands, Kate, van der Werf, Paul, Driver, Simon, Dunne, Loretta, Dye, Simon, Furlanetto, Cristina, Ivison, R. J., Maddox, Steve, Robotham, Aaron, Smith, Matthew W. L., Taylor, Edward N., Valiante, Elisabetta, Wright, Angus, Cigan, Philip, De Zotti, Gianfranco, Jarvis, Matt J., Marchetti, Lucia, Michałowski, Michał J., Phillipps, Steven, Viaene, Sebastien, Vlahakis, Catherine
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Sprache:eng
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Zusammenfassung: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 star-forming 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 
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stx2548