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The Angular Momentum of Brightest Cluster Galaxies

Brough, S. ; Tran, K.-V ; von der Linden, A.

In: Proceedings of the International Astronomical Union, 2012, vol. 8, no. S295, p. 229-229

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    Titel
    • The Angular Momentum of Brightest Cluster Galaxies
    Autor
    • Brough, S.. Australian Astronomical Observatory, PO Box 915, North Ryde, NSW 1670, Australia
    • Tran, K.-V. George P. & Cynthia W. Mitchell Institute for Fundamental Physics & Astronomy, Department of Physics & Astronomy, Texas A&M University, College Station, TX 77843, USA
    • von der Linden, A.. Kavli Institute of Particle Astrophysics & Cosmology (KIPAC), Stanford University, 452 Lomita Mall, Stanford, CA 94305, USA
    Dokumententyp
    • Postprint
    Sprache
    • Englisch
    Veröffentlicht in
    • Proceedings of the International Astronomical Union, 2012, vol. 8, no. S295, p. 229-229. Cambridge University Press
    Andere elektronische Ausgabe
    OAI-PMH-ID
    • oai:doc.rero.ch:291573
    Summary
    Massive Brightest Cluster Galaxies (BCGs) are observed to have a range of angular momenta, suggesting a variety of merging histories