Galaxies and Star Clusters – From the Computer to the Real World

G01 New evidence for a connection between massive black holes and ULX

G02 Long-Term Evolution of Massive Black Hole Binaries

G03 NBODY Meets Stellar Population Synthesis

G04 N-body modelling of real globular star clusters

G05 Fokker-Planck rotating models of globular clusters with black hole

G06 Observational Manifestation of chaos in spiral galaxies: quantitative analysis and qualitative explanation

G07 GRAPE Clusters: Beyond the Million-Body Problem

G08 Orbital decay of star clusters and Massive Black Holes in cuspy galactic nuclei

G09 An Edge-on Disk Galaxy Catalog

G10 Complexes of open clusters in the Solar neighborhood

G11 Search for and investigation of new stellar clusters using the data from huge stellar catalogues

G12 Computing 2D images of 3D galactic disk models

G13 Outer Pseudoring in the Galaxy

G14 Where are tidal-dwarf galaxies?

G15 Ultra compact dwarf galaxies in nearby clusters

G16 Impact of an Accretion Disk on the Structure of a stellar cluster in active galactic nuclei

G17 Order and Chaos in the edge-on profiles of disk galaxies

G18 On the stability of OB-star configurations in the Orion Nebula cluster

G19 Older stars captured in young star clusters by cloud collapse

G20 General features of the population of open clusters within 1 kpc from the Sun

G21 Unstable modes in thin stellar disks

G22 From Newton to Einstein – Dynamics of N-body systems

G23 On the relation between the maximum stellar mass and the star cluster mass