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Kinematics of globular cluster systems in galaxy mergers

Published online by Cambridge University Press:  01 July 2007

Christopher C. Hayward ,
T. J. Cox  and
Lars Hernquist
Christopher C. Hayward
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA email: [email protected], [email protected], [email protected]
T. J. Cox
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA email: [email protected], [email protected], [email protected]
Lars Hernquist
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA email: [email protected], [email protected], [email protected]
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Abstract

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We use numerical simulations to study how the spatial distribution and kinematics of globular cluster systems (GCS) are affected by galaxy mergers. Each progenitor galaxy is given a GCS modeled after the Galactic GCS. We then study how a major merger affects the spatial distribution and kinematics of the GCS. Here we present our methodology. Future work will investigate the effects of varying galaxy parameters, merger orbital parameters, and initial GCS number density profile and kinematics. We hope to be able to extract information about the merger history of a galaxy from observations of its GCS spatial distribution and kinematics.

Keywords

galaxies: formationgalaxies: evolutiongalaxies: kinematics and dynamicsgalaxies: star clusters(Galaxy:) globular clusters: generalmethods: n-body simulations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S245: Formation and Evolution of Galaxy Bulges , July 2007 , pp. 77 - 78
Copyright
Copyright © International Astronomical Union 2008

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