Add to ORKGA short story of dark matter as an example of a scientific revolution is given. The characteristics of stellar populations are compared with those of dark halos. The mean mass-to-luminosity ratio of stellar populations is found to be 4 in Solar units. Dark matter around galaxies, and in groups, clusters and voids is discussed. Modern data suggest that the overall density of matter in the Universe is 0.3 +- 0.1, about 80% of this matter is non-baryonic dark matter, and about 20% is baryonic, mostly in the form of hot intra-cluster and intragroup gas, the rest in stellar populations of galaxies. The Universe is dominated by dark energy (cosmological constant) term
The balance of evidence indicates that individual galaxies and groups or clusters of galaxies are em...
A wealth of recent observational studies shows the dark matter in the Milky Way to have the followin...
These lectures cover various aspects of the statistical description of cosmological density fields. ...
Dark matter in galaxies, its abundance, and its distribution remain a subject of long-standing discu...
Observations in the optical, in X-rays, and gravitational lensing of galaxies, clusters of galaxies,...
The dynamical masses of dwarf-spheroidals, spiral and elliptical galaxies, dwarf irregular binaries,...
We investigate how the properties of the dark matter and baryons in groups and clusters of galaxies ...
Rich clusters of galaxies, the largest virialized systems known, provide a powerful tool for the stu...
This thesis addresses the distributions of baryonic matter on three scales: the outskirts of the gas...
Contribution from the students of the 4th CERNCLAF School of High-Energy Physics who participated in...
There is evidence that dark matter constitutes a majority of the Universe's matter content. Yet, we ...
During the last few decades, it has been discovered that most of the material in the Universe is inv...
The existence of Dark Matter (DM) has been known since the 30's of the last century. The first cogni...
When interpreted within the standard framework of Newtonian gravity and dynamics, the kinematics of ...
To account for the source of dark matter(energy),a theory based on gravitation is developed in this ...
The balance of evidence indicates that individual galaxies and groups or clusters of galaxies are em...
A wealth of recent observational studies shows the dark matter in the Milky Way to have the followin...
These lectures cover various aspects of the statistical description of cosmological density fields. ...
Dark matter in galaxies, its abundance, and its distribution remain a subject of long-standing discu...
Observations in the optical, in X-rays, and gravitational lensing of galaxies, clusters of galaxies,...
The dynamical masses of dwarf-spheroidals, spiral and elliptical galaxies, dwarf irregular binaries,...
We investigate how the properties of the dark matter and baryons in groups and clusters of galaxies ...
Rich clusters of galaxies, the largest virialized systems known, provide a powerful tool for the stu...
This thesis addresses the distributions of baryonic matter on three scales: the outskirts of the gas...
Contribution from the students of the 4th CERNCLAF School of High-Energy Physics who participated in...
There is evidence that dark matter constitutes a majority of the Universe's matter content. Yet, we ...
During the last few decades, it has been discovered that most of the material in the Universe is inv...
The existence of Dark Matter (DM) has been known since the 30's of the last century. The first cogni...
When interpreted within the standard framework of Newtonian gravity and dynamics, the kinematics of ...
To account for the source of dark matter(energy),a theory based on gravitation is developed in this ...
The balance of evidence indicates that individual galaxies and groups or clusters of galaxies are em...
A wealth of recent observational studies shows the dark matter in the Milky Way to have the followin...
These lectures cover various aspects of the statistical description of cosmological density fields. ...