The Starlab Environment for Dense Stellar Systems
Traditionally, a simulation of a dense stellar system required choosing an initial model, running an integrator, and analyzing the output.
36 indexed results
Traditionally, a simulation of a dense stellar system required choosing an initial model, running an integrator, and analyzing the output.
We present two types of meta-algorithm that can greatly improve the accuracy of existing algorithms for integrating the equations of
We have analyzed the far UV-spectrum of the globular cluster M79. We show that the nearly Gaussian mass distribution of
Bipolar outflows are known to be present in many disk-accreting astrophysical systems. In disk-dominated cataclysmic variables, these outflows are responsible
The XA region of the Cygnus Loop is a complex zone of radiative and nonradiative shocks interacting with interstellar clouds.
We have implemented a parallel version of the Barnes-Hut 3-D N-body tree algorithm under PVM 3.2.5, adopting an SPMD paradigm.
Composite spectra derived from HST observations of moderate redshift (z~1) quasars show that the peak of the spectral energy distribution
Much of the far-UV emission from elliptical galaxies is thought to arise from extreme horizontal branch stars and related objects.
[Abridged] The interaction rates of dark-matter halos and subhalos, are computed using high-resolution cosmological N-body simulations of the Lambda-CDM model.
We present the summary of the theoretical aspects and algorithms used in an undergraduate (JRG) summer project based on numerical
I describe here the performances of a parallel treecode with individual particle timesteps. The code is based on the Barnes-Hut
Recent observational and theoretical developments concerning the origin of the ultraviolet emission from ellipticals are reviewed and discussed,with particular, reference