->PUBLICATION LIST
Physics of the Intersteller Medium (ISM)
- Evolution of the ISM as non-equilibrium phenomena
- Phase transition, spinodal decomposition and pattern formation of the ISM
Galaxy formation
- Semi-analytic modelling of galaxy formation
- Evolution of cluster galaxies
-> e.g. ram-pressure stripping in the intracluster medium (ICM)
- Physical understanding of some phenomenological laws of cluster
galaxies
-> e.g. color-magnitude relation, morphology-density relation, etc.
- Effects of the UV background raditaion on galaxy formation
- Formation and evolution of dwarf galaxies
- NuGC(Numerical Galaxy Catalo) home page
QSO absorption line systems
- Unified interpretation of damped Ly-alpha systems with galaxy evolution
QSO formation
- Semi-analytic modelling of QSO formation
- Galaxies and QSO environments
Observational cosmology
- Galaxy number counts in a galaxy formation model
High energy astrophysics
- Gamma-ray emission from forming haloes
Formation and evolution of the large-scale structure of the Universe
- Mass function based on the density fluctuation field in the early Universe
- Structure formation in non-Gaussian initial conditions
- Formation histories of dark matter halos
- Angular momentum evolution of dark matter halos
Future work
- Galaxy evolution based on the evolution of the interstellar medium (ISM)
- Thermal evolution of the ICM
- Growth of planetesimals in proto-planetary disks
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