Add to ORKGI suggest that the bulk of the "young", second-parameter globular clusters (SPGCs) observed in the outer halo of our Galaxy and recently found in other massive spiral of the Local Group (LG), M33, may have originated due to mass outflow from M31 and subsequent accretion of gas on the Galaxy and M33 in the early epoch
We examine various implications from a dynamical and chemical model of globular clusters (GCs), whic...
Presently unaccounted but quite probable "chemical factor" may be responsible for the formation of o...
Large galaxies grow through the accumulation of dwarf galaxies(1,2). In principle it is possible to ...
We suggest that the majority of the “young”, so–called “second parameter” globular clusters (SPGCs...
We find that the globular cluster (GC) systems of the Milky Way and of our neighboring spiral galaxy...
We find that the globular cluster (GC) systems of the Milky Way and of our neighboring spiral galaxy...
We find that the globular cluster (GC) systems of the Milky Way and of our neighboring spiral galaxy...
We review the properties of globular clusters (GCs) which make them useful for studying the Galactic...
Two recent observations regarding the halo of M33 seem to contradict each other. First, the star clu...
We have carried out a large grid of N-body simulations in order to investigate if mass loss as a res...
Globular clusters are often assumed to be good tracers of major star formation episodes in their hos...
Despite the rapid observational progress in the study of young massive star clusters, the formation ...
We propose and investigate a new formation mechanism for globular clusters in which they form within...
I assess the similarities and differences between the star-formation modes in quiescent spiral galax...
Many scenarios for the origin of the chemical anomalies observed in globular clusters (GCs; i.e., mu...
We examine various implications from a dynamical and chemical model of globular clusters (GCs), whic...
Presently unaccounted but quite probable "chemical factor" may be responsible for the formation of o...
Large galaxies grow through the accumulation of dwarf galaxies(1,2). In principle it is possible to ...
We suggest that the majority of the “young”, so–called “second parameter” globular clusters (SPGCs...
We find that the globular cluster (GC) systems of the Milky Way and of our neighboring spiral galaxy...
We find that the globular cluster (GC) systems of the Milky Way and of our neighboring spiral galaxy...
We find that the globular cluster (GC) systems of the Milky Way and of our neighboring spiral galaxy...
We review the properties of globular clusters (GCs) which make them useful for studying the Galactic...
Two recent observations regarding the halo of M33 seem to contradict each other. First, the star clu...
We have carried out a large grid of N-body simulations in order to investigate if mass loss as a res...
Globular clusters are often assumed to be good tracers of major star formation episodes in their hos...
Despite the rapid observational progress in the study of young massive star clusters, the formation ...
We propose and investigate a new formation mechanism for globular clusters in which they form within...
I assess the similarities and differences between the star-formation modes in quiescent spiral galax...
Many scenarios for the origin of the chemical anomalies observed in globular clusters (GCs; i.e., mu...
We examine various implications from a dynamical and chemical model of globular clusters (GCs), whic...
Presently unaccounted but quite probable "chemical factor" may be responsible for the formation of o...
Large galaxies grow through the accumulation of dwarf galaxies(1,2). In principle it is possible to ...