Name	E_mail_Address	Scientific_Session	Contribution_type	Title	Authors_affiliations	Abstract	
Spurzem, Rainer	spurzem@ari.uni-heidelberg.de	EAS Symp.6:Dynamics of Galaxies and Galactic Nuclei.	oral	Post-Newtonian Dynamics in Dense Stellar Systems	R. Spurzem (1), D. Merritt (2), Peter Berczik (1),
Ingo Berentzen (1), Miguel Preto (1), Jonathan Downing(1); 1) Astron. Rechen-Inst. Zentrum Astron. Univ. Heidelberg, Germany, 2)Rochester Inst. of Technology, Rochester, New York, USA 	Dense stellar systems (star clusters and galactic nuclei) are some of the most
promising sources 
of gravitational waves since black holes may form and grow in them. In the
talk I will describe how 
relativistic dynamics is included in $N$-body simulations of such systems, and
discuss examples how we 
model sources in different wavelength regimes, showing results from triple and
binary black holes in 
galactic nuclei, and giving an outlook to projected work for star
clusters. Also I\'ll explain how these 
theoretical activities are embedded into collaborative programs with
gravitational wave observatories, 
such as the VESF (Virgo-EGO science collaboration) and the German LISA cooperation.