Add to ORKGWe have performed a set of realistic N-body simulations of the evolution of multi-mass star clusters in external tidal fields. Our clusters started with the same initial mass-functions, but varying particle numbers, orbital types and density profiles
The distribution of stars and stellar remnants (white dwarfs, neutron stars, and black holes) within...
The distribution of stars and stellar remnants (white dwarfs, neutron stars, and black holes) within...
The distribution of stars and stellar remnants (white dwarfs, neutron stars, and black holes) within...
We present N-body simulations of realistic globular clusters containing initial mass function in the...
We report the results of a large set of N-body calculations aimed at studying the evolution of multi...
The evolution of the global stellar mass function of star clusters is studied based on a large set o...
The evolution of the global stellar mass function of star clusters is studied based on a large set o...
We present the results of a survey of $N$-body simulations aimed at studying the effects of the long...
Context. The dynamical escape of stars from star clusters affects the shape of the stellar mass func...
In this paper, we compare the mass function slopes of Galactic globular clusters recently determined...
The dynamical escape of stars from star clusters affects the shape of the stellar mass function (MF)...
The dynamical escape of stars from star clusters affects the shape of the stellar mass function (MF)...
As we enter a golden age for studies of internal kinematics and dynamics of Galactic globular cluste...
The dynamical escape of stars from star clusters affects the shape of the stellar mass function (MF)...
The dynamical escape of stars from star clusters affects the shape of the stellar mass function (MF)...
The distribution of stars and stellar remnants (white dwarfs, neutron stars, and black holes) within...
The distribution of stars and stellar remnants (white dwarfs, neutron stars, and black holes) within...
The distribution of stars and stellar remnants (white dwarfs, neutron stars, and black holes) within...
We present N-body simulations of realistic globular clusters containing initial mass function in the...
We report the results of a large set of N-body calculations aimed at studying the evolution of multi...
The evolution of the global stellar mass function of star clusters is studied based on a large set o...
The evolution of the global stellar mass function of star clusters is studied based on a large set o...
We present the results of a survey of $N$-body simulations aimed at studying the effects of the long...
Context. The dynamical escape of stars from star clusters affects the shape of the stellar mass func...
In this paper, we compare the mass function slopes of Galactic globular clusters recently determined...
The dynamical escape of stars from star clusters affects the shape of the stellar mass function (MF)...
The dynamical escape of stars from star clusters affects the shape of the stellar mass function (MF)...
As we enter a golden age for studies of internal kinematics and dynamics of Galactic globular cluste...
The dynamical escape of stars from star clusters affects the shape of the stellar mass function (MF)...
The dynamical escape of stars from star clusters affects the shape of the stellar mass function (MF)...
The distribution of stars and stellar remnants (white dwarfs, neutron stars, and black holes) within...
The distribution of stars and stellar remnants (white dwarfs, neutron stars, and black holes) within...
The distribution of stars and stellar remnants (white dwarfs, neutron stars, and black holes) within...