We present results from the largest numerical simulation of star formation to\nresolve the fragmentation process down to the opacity limit. The simulation\nfollows the collapse ...
We investigate the physics of gas accretion in young stellar clusters.\nAccretion in clusters is a dynamic phenomenon as both the stars and the gas\nrespond to the same gravitat...
We present results from the first hydrodynamical star formation calculation to demonstrate that brown dwarfs are a natural and frequent product of the collapse and fragmentation...
We present results from a numerical simulation of gas accretion in a cluster containing 1000 stars. The accretion forces the cluster to contract, leading to the development of a...
Submillimetre HCO+(J = 4 − 3) mapping observations of the immediate environs of the infrared source IRS 7 in Corona Australis have provided corroborative evidence for the existe...
We investigate the effects of gas accretion on small clusters of young stars. The evolution of clusters containing 3–10 stars and between 0.1 and 90 per cent of their masses in ...
We present a simple physical mechanism that can account for the observed stellar mass spectrum for masses $\ms \simgreat 0.5 \solm$. The model depends solely on the competitive ...
We present a model for the formation of massive ($M > 10 M_\odot$) stars through accretion-induced collisions in the cores of embedded dense stellar clusters. This model circumv...
h-index: Number of publications with at least h citations each.