Add to ORKGA viable scenario for globular cluster formation is suggested in CDM model. In this scenario the smaller scale fluctuations superposed on proto-galaxy will form proto-dwarf-galaxies. In their multi-phase ISM the warm Clouds, which are thermally stable and gravitationally marginally stable with appropriate masses and metallicities, might be the proper progenitors of GCs. In the virialization of a proto-galaxy, these dwarf galaxies will acquire kinetic energy and collide with each other. As strong external disturbances, these collisions will cause a short timescale thermal instability, and further stimulate gravitational instability which is necessary for the transformation of progenitors into GCs.Mathematics, AppliedMathematicsSCI(E)0ARTI...
The authors propose an evolutionary model for dwarf galaxies in which initially metal-poor gas-rich ...
Accepted for publication on ApJWe study the evolution of dwarf (L_H < 10^{9.6} L_Ho) star forming an...
We apply the semi-analytical galaxy formation code of Cole et al. to investigate the formation of gl...
A Viable scenario for globula r cluster formation is suggested in CDM model.In this scenario the sma...
We propose a self-consistent model for globular cluster formation in, but not limited to, our Galaxy...
Galaxy clusters contain a large population of low-mass dwarf elliptical galaxies whose exact origin ...
We present a hydrodynamical simulation at sub-parsec and few-solar-mass resolution of a merger betwe...
Many models of globular cluster formation assume the presence of cold dense clouds in early universe...
We first review the results of the tidal stirring model for the transformation of gas-rich dwarf irr...
We investigate a scenario where the formation of globular clusters (GCs) is triggered by high-speed ...
We investigate a scenario where the formation of globular clusters (GCs) is triggered by high-speed ...
Our numerical simulations first demonstrate that the pressure of ISM in a major merger becomes so hi...
I summarize the known properties of globular cluster systems. Often the globular cluster systems of ...
Using a state-of-the-art cosmological simulation of merging proto-galaxies at high redshift from the...
We revise the scenario of the formation of Galactic globular clusters (GCs) by adding the observed d...
The authors propose an evolutionary model for dwarf galaxies in which initially metal-poor gas-rich ...
Accepted for publication on ApJWe study the evolution of dwarf (L_H < 10^{9.6} L_Ho) star forming an...
We apply the semi-analytical galaxy formation code of Cole et al. to investigate the formation of gl...
A Viable scenario for globula r cluster formation is suggested in CDM model.In this scenario the sma...
We propose a self-consistent model for globular cluster formation in, but not limited to, our Galaxy...
Galaxy clusters contain a large population of low-mass dwarf elliptical galaxies whose exact origin ...
We present a hydrodynamical simulation at sub-parsec and few-solar-mass resolution of a merger betwe...
Many models of globular cluster formation assume the presence of cold dense clouds in early universe...
We first review the results of the tidal stirring model for the transformation of gas-rich dwarf irr...
We investigate a scenario where the formation of globular clusters (GCs) is triggered by high-speed ...
We investigate a scenario where the formation of globular clusters (GCs) is triggered by high-speed ...
Our numerical simulations first demonstrate that the pressure of ISM in a major merger becomes so hi...
I summarize the known properties of globular cluster systems. Often the globular cluster systems of ...
Using a state-of-the-art cosmological simulation of merging proto-galaxies at high redshift from the...
We revise the scenario of the formation of Galactic globular clusters (GCs) by adding the observed d...
The authors propose an evolutionary model for dwarf galaxies in which initially metal-poor gas-rich ...
Accepted for publication on ApJWe study the evolution of dwarf (L_H < 10^{9.6} L_Ho) star forming an...
We apply the semi-analytical galaxy formation code of Cole et al. to investigate the formation of gl...