Hostname: page-component-78c5997874-ndw9j Total loading time: 0 Render date: 2024-11-13T05:33:51.930Z Has data issue: false hasContentIssue false
  • English
  • Français

Slow Evolution of a System of Satellites Induced by Dynamical Friction

Published online by Cambridge University Press:  01 September 2007

Serena E. Arena  and
Giuseppe Bertin
Serena E. Arena
Affiliation:
Dipartimento di Fisica, Università degli Studi di Milano, via Celoria 16, I-20133 Milano, Italy E-mail: serena.arena@unimi.it, giuseppe.bertin@unimi.it
Giuseppe Bertin
Affiliation:
Dipartimento di Fisica, Università degli Studi di Milano, via Celoria 16, I-20133 Milano, Italy E-mail: serena.arena@unimi.it, giuseppe.bertin@unimi.it
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The evolution induced by dynamical friction on a spherical shell of rigid satellites interacting directly with the particles sampling the host elliptical galaxy is followed by means of N-body simulations for a variety of shell–galaxy configurations.

Keywords

stellar dynamicsmethods: n-body simulationsgalaxies: kinematics and dynamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S246: Dynamical Evolution of Dense Stellar Systems , September 2007 , pp. 423 - 424
Copyright
Copyright © International Astronomical Union 2008

References

Arena, S. E., Bertin, G., Liseikina, T., & Pegoraro, F. 2006, A&A, 453, 9Google Scholar
Arena, S.E., & Bertin, G. 2007, A&A, 463, 921Google Scholar
Arena, S. E. 2007, Ph.D. Thesis, Università degli Studi di Milano, MilanoGoogle Scholar
Bertin, G., Liseikina, T., & Pegoraro, F. 2003, A&A, 405, 73Google Scholar
Trenti, M. 2005, Ph.D. Thesis, Scuola Normale Superiore, PisaGoogle Scholar
Trenti, M., & Bertin, G. 2005, A&A, 429, 161Google Scholar