Probing the kinematics of early-type galaxy halos using planetary nebulae

L. Coccato*, P. Gerhard, M. Arnaboldi, P. Das, N. G. Douglas, K. Kijken, M. R. Merrifield, N. R. Napolitano, E. Noordermeer, A. J. Romanowsky, M. Capaccioli, A. Cortesi, F. De Lorenzi, K. C. Freeman

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    2 Citations (Scopus)

    Abstract

    We present first results of a study of the halo kinematics for a sample of early type galaxies using planetary nebulae (PNe) as kinematical tracers. PNe allow to extend up to several effective radii (Re) the information from absorption line kinematics (confined to within 1 or 2Re), providing valuable information and constraints for merger simulations and galaxy formation models. We find that the specific angular momentum per unit mass has a more complex radial dependence when the halo region is taken into account and that the halo velocity dispersion is related to the total galaxy luminosity, isophotal shape, and number of PNe per unit of luminosity .

    Original languageEnglish
    Pages (from-to)912-915
    Number of pages4
    JournalAstronomische Nachrichten
    Volume329
    Issue number9-10
    DOIs
    Publication statusPublished - Dec 2008

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