68 citations · 110 across the 4 of their papers we have counts for
4 papers
Massive star cluster formation I. High star formation efficiency while resolving feedback of individual stars
Brooke Polak, Mordecai-Mark Mac Low, Ralf S. Klessen +11
The mode of star formation that results in the formation of globular clusters and young massive clusters is difficult to constrain through observations. We present models of massiv…
Merger rates of black hole binaries: prospects for gravitational wave detectors
Simon Portegies Zwart, Stephen McMillan
Mergers of black-hole binaries are expected to release large amounts of energy in the form of gravitational radiation. However, binary evolution models predict merger rates too low…
Gravitational Radiation from the Coalescence of Binary Neutron Stars: Effects Due to the Equation of State, Spin, and Mass Ratio
Xing Zhuge, Joan M. Centrella, Stephen L. W. McMillan
We calculate the gravitational radiation produced by the coalescence of inspiraling binary neutron stars in the Newtonian regime using 3-dimensional numerical simulations. The star…
Gravothermal Expansion in an -Body System
Douglas C. Heggie, Shogo Inagaki, Stephen L. W. McMillan
This paper describes the numerical evolution of an -body system with a slight ``temperature inversion''; i.e. the maximum velocity dispersion occurs not at the centre but furthe…