The Galactic Bulge can uniquely be studied from large samples of individual stars and is
therefore of prime importance for understanding the stellar population structure of bulges in …

The dynamics of interacting galaxies as observed in the present epoch is reviewed. Topics
discussed include numerical methods for modeling galactic interactions, the signatures of …

Smoothed particle hydrodynamics ADS Classic is now deprecated. It will be completely
retired in October 2019. This page will automatically redirect to the new ADS interface at …

This book discusses in detail all the relevant numerical methods for the classical N-body
problem. It demonstrates how to develop clear and elegant algorithms for models of …

Introducing the dragon simulation project, we present direct N-body simulations of four
massive globular clusters (GCs) with 106 stars and 5 per cent primordial binaries at a high …

Accurate direct N-body simulations help to obtain detailed information about the dynamical
evolution of star clusters. They also enable comparisons with analytical models and Fokker …

Planetary accretion from planetesimals to protoplanets is investigated using three-
dimensional N-body simulations. The effect of gas drag due to solar nebula is included and …

Recent observations have shown that globular clusters contain a significant binary
population. This is a dramatic change from the conventional view of even a decade ago …

Galactic globular clusters, which are ancient building blocks of our Galaxy, represent a very
interesting family of stellar systems in which some fundamental dynamical processes have …

We have simulated the formation of an X-ray cluster in a cold dark matter universe using 12
different codes. The codes span the range of numerical techniques and implementations …