Future space and ground-based survey programmes will produce an impressiveamount of photometric data. The GAIA space mission will map the complete skydown to mag V=20 and produce time series for about 1 billion stars. Surveyinstruments as the International Liquid Mirror Telescope will observe slices ofthe sky down to magnitude V=23. In both experiments, the opportunity exists todiscover a huge amount of variable stars. A prediction of the expected totalnumber of variable stars and the number of variables in specific subgroups isgiven
We have developed a consistent analytical model to describe the observed evolution of the quasar lum...
At OAB we were, during the year 1998, deeply involved in planning two important space missions for w...
We use linear and quasi-linear perturbation theory to analyse cold dark matter models of structure f...
Two studies have recently reported the discovery of pronounced Halo substructure in the Sloan Digita...
Measurements of heavy quark production at a possible future $ep$ facility, THERA, would provide valu...
We re-examine the assembly history of field spheroidals as a potentially powerful discriminant of ga...
Age dating starbursts is an exercise with many caveats. We attempt to summarise a discussion session...
One hundred years after the eruption of GK Per and the detection of oscillations in its light curve ...
Near-infrared (NIR) K' images of a sample of five low surface brightness disc galaxies (LSBGs) were ...
It has become increasingly apparent that traditional hydrodynamical simulations of galaxy clusters a...
Gamma ray emission lines resulting from accelerated particle bombardment of ambient gas can serve as...
We demonstrate that the Biermann battery mechanism for the creation of large scale magnetic fields c...
Upcoming weak lensing surveys on wide fields will provide the opportunity to reconstruct the structu...
The time evolution of wave packets in a harmonic oscillator potential is studied. Some new results f...
We have discovered polarized broad emission lines in five type 2 Seyfert galaxies (NGC 424, NGC 591,...
We have developed a consistent analytical model to describe the observed evolution of the quasar lum...
At OAB we were, during the year 1998, deeply involved in planning two important space missions for w...
We use linear and quasi-linear perturbation theory to analyse cold dark matter models of structure f...
Two studies have recently reported the discovery of pronounced Halo substructure in the Sloan Digita...
Measurements of heavy quark production at a possible future $ep$ facility, THERA, would provide valu...
We re-examine the assembly history of field spheroidals as a potentially powerful discriminant of ga...
Age dating starbursts is an exercise with many caveats. We attempt to summarise a discussion session...
One hundred years after the eruption of GK Per and the detection of oscillations in its light curve ...
Near-infrared (NIR) K' images of a sample of five low surface brightness disc galaxies (LSBGs) were ...
It has become increasingly apparent that traditional hydrodynamical simulations of galaxy clusters a...
Gamma ray emission lines resulting from accelerated particle bombardment of ambient gas can serve as...
We demonstrate that the Biermann battery mechanism for the creation of large scale magnetic fields c...
Upcoming weak lensing surveys on wide fields will provide the opportunity to reconstruct the structu...
The time evolution of wave packets in a harmonic oscillator potential is studied. Some new results f...
We have discovered polarized broad emission lines in five type 2 Seyfert galaxies (NGC 424, NGC 591,...
We have developed a consistent analytical model to describe the observed evolution of the quasar lum...
At OAB we were, during the year 1998, deeply involved in planning two important space missions for w...
We use linear and quasi-linear perturbation theory to analyse cold dark matter models of structure f...