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The ATLAS3D project - XXVII. Cold gas and the colours and ages of early-type galaxies

Research output: Contribution to journalArticle

  • Lisa M. Young
  • Nicholas Scott
  • Paolo Serra
  • Katherine Alatalo
  • Estelle Bayet
  • Leo Blitz
  • Maxime Bois
  • Frédéric Bournaud
  • Martin Bureau
  • Alison F. Crocker
  • Michele Cappellari
  • Roger L. Davies
  • Timothy A. Davis
  • P. T. de Zeeuw
  • Pierre-Alain Duc
  • Eric Emsellem
  • Davor Krajnović
  • Harald Kuntschner
  • Richard M. McDermid
  • Raffaella Morganti
  • Thorsten Naab
  • Tom Oosterloo
  • Marc Sarzi
  • Anne-Marie Weijmans

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http://adsabs.harvard.edu/abs/2014MNRAS.444.3408Y
http://mnras.oxfordjournals.org/content/444/4/3408.abstract?sid=364230fc-8062-4958-bdd2-2c7882007de2
Original languageEnglish
Pages (from-to)3408-3426
JournalMonthly Notices of the Royal Astronomical Society
Volume444
Issue number4
Early online date17 Sep 2014
DOIs
StatePublished - 1 Nov 2014

Abstract

We present a study of the cold gas contents of the ATLAS3D early-type galaxies, in the context of their optical colours, near-ultraviolet colours and Hβ absorption line strengths. Early-type (elliptical and lenticular) galaxies are not as gas poor as previously thought, and at least 40 per cent of local early-type galaxies are now known to contain molecular and/or atomic gas. This cold gas offers the opportunity to study recent galaxy evolution through the processes of cold gas acquisition, consumption (star formation) and removal. Molecular and atomic gas detection rates range from 10 to 34 per cent in red sequence early-type galaxies, depending on how the red sequence is defined, and from 50 to 70 per cent in blue early-type galaxies. Notably, massive red sequence early-type galaxies (stellar masses >5 × 1010 M⊙, derived from dynamical models) are found to have H I masses up to M(H I)/M* ˜ 0.06 and H2 masses up to M(H2)/M* ˜ 0.01. Some 20 per cent of all massive early-type galaxies may have retained atomic and/or molecular gas through their transition to the red sequence. However, kinematic and metallicity signatures of external gas accretion (either from satellite galaxies or the intergalactic medium) are also common, particularly at stellar masses ≤5 × 1010 M⊙, where such signatures are found in ˜50 per cent of H2-rich early-type galaxies. Our data are thus consistent with a scenario in which fast rotator early-type galaxies are quenched former spiral galaxies which have undergone some bulge growth processes, and in addition, some of them also experience cold gas accretion which can initiate a period of modest star formation activity. We discuss implications for the interpretation of colour-magnitude diagrams.

    Research areas

  • galaxies: elliptical and lenticular, cD, galaxies: evolution, galaxies: ISM, galaxies: structure, radio lines: galaxies

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