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Towards a New Classification of Early-type Galaxies: An Integral-field View

  • J. Falcon-Barroso
  • , R. Bacon
  • , M. Cappellari
  • , R.L. Davies
  • , P.T. de Zeeuw
  • , E. Emsellem
  • , D. Krajnovic
  • , H. Kuntschner
  • , R.M. McDermid
  • , R.F. Peletier
  • , M. Sarzi
  • , G. van de Ven

    Research output: Chapter in Book/Report/Conference proceedingConference contribution

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    Abstract

    In this proceedings paper we make use of the two-dimensional stel- lar kinematics of a representative sample of E and S0 galaxies obtained with the SAURON integral-field spectrograph to reveal that early-type galaxies appear in two broad flavors, depending on whether they exhibit clear large-scale rotation or not. We measure the level of rotation via a new parameter (λR) and use it as a basis for a new kinematic classification that separates early-type galaxies into slow and fast rotators. With the aid of broad-band imaging we will reinforce this finding by comparing our kinematic results to the photometric properties of these two classes.
    Original languageEnglish
    Title of host publicationIn: Pathways Through an Eclectic Universe - ASP Conf Series 390
    PublisherAstronomical Society of the Pacific
    Pages227-231
    ISBN (Print)978-1-58381-651-6, 978-1-58381-650-9
    Publication statusPublished - 2008

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