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The Angular Momentum of Brightest Cluster Galaxies

Published online by Cambridge University Press:  17 July 2013

S. Brough ,
K.-V. Tran  and
A. von der Linden
S. Brough
Affiliation:
Australian Astronomical Observatory, PO Box 915, North Ryde, NSW 1670, Australia
K.-V. Tran
Affiliation:
George P. & Cynthia W. Mitchell Institute for Fundamental Physics & Astronomy, Department of Physics & Astronomy, Texas A&M University, College Station, TX 77843, USA Institute for Theoretical Physics, University of Zurich, CH 8057, Switzerland
A. von der Linden
Affiliation:
Kavli Institute of Particle Astrophysics & Cosmology (KIPAC), Stanford University, 452 Lomita Mall, Stanford, CA 94305, USA
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Abstract

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Massive Brightest Cluster Galaxies (BCGs) are observed to have a range of angular momenta, suggesting a variety of merging histories.

Keywords

galaxies: elliptical and lenticularcDgalaxies: kinematics and dynamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S295: The intriguing life of massive galaxies , August 2012 , pp. 229
Copyright
Copyright © International Astronomical Union 2013 

References

Brough, S., et al. 2011, MNRAS, 413, 1236Google Scholar
Collins, C. A., et al. 2009, Nature, 458, 603CrossRefGoogle Scholar
Lidman, C., et al. 2012, MNRAS, 427, 550CrossRefGoogle Scholar