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Slide 1 Close encounters between stars and Massive Black Holes Clovis Hopman Weizmann Institute of Science Israel Advisor: Tal Alexander Slide 2 Tidally powered stars in…

Slide 1 Formation of an IMF-Cluster in a Filamentary Layer Collaborators: F. Adams (Michigan), L. Allen (CfA), R. Gutermuth (CfA), J. Jørgensen (CfA), S. T. Megeath (Toledo)…

Timestepping and Parallel Computing in Highly Dynamic N-body Systems Joachim Stadel [email protected] University of Zürich Institute for Theoretical Physics Astrophysical…

The Swansong of Stars Orbiting Massive Black Holes Clovis Hopman Weizmann Institute of Science Israel Advisor: Tal Alexander Dissipative stellar processes near Massive Black…

The new estimates of the IMF in compact stellar systems A Novel Technique for the Determination of IMF at Low Masses: A Few Results for Galaxies with Old Stellar Populations…

The Initial Mass Function in Clusters Bruce G. Elmegreen IBM T.J. Watson Research Center Yorktown Hts., NY [email protected] May 9, 2006 Salpeter ‘55 slope=-1.35 The IMF…

Close encounters between stars and Massive Black Holes Clovis Hopman Weizmann Institute of Science Israel Advisor: Tal Alexander Dissipative stellar processes near Massive…

Minerals: how do they form in planets? Minerals: how do they form in planets? By: Josh Gates and Michael Parris The Rocky Inner Planets The four inner planets are composed…

Timestepping and Parallel Computing in Highly Dynamic N-body Systems Joachim Stadel [email protected] University of Zürich Institute for Theoretical Physics Astrophysical…