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The Science Case for the Planet Formation Imager (PFI)
Stefan Kraus, John Monnier, Tim Harries +16
Among the most fascinating and hotly-debated areas in contemporary astrophysics are the means by which planetary systems are assembled from the large rotating disks of gas and dust…
Two fluid dust and gas mixtures in SPH: A semi-implicit approach
Pablo Loren-Aguilar, Matthew R. Bate
A method to avoid the explicit time integration of small dust grains in the two fluid gas/dust smoothed particle hydrodynamics (SPH) approach is proposed. By assuming a very simple…
The statistical properties of stars and their dependence on metallicity: the effects of opacity
Matthew R. Bate
We report the statistical properties of stars and brown dwarfs obtained from four radiation hydrodynamical simulations of star cluster formation that resolve masses down to the opa…
The Spatial Structure of Young Stellar Clusters. I. Subclusters
Michael A. Kuhn, Eric D. Feigelson, Konstantin V. Getman +9
The clusters of young stars in massive star-forming regions show a wide range of sizes, morphologies, and numbers of stars. Their highly subclustered structures are revealed by the…
Star Cluster Formation and Feedback
Mark R. Krumholz, Matthew R. Bate, Hector G. Arce +6
Stars do not generally form in isolation. Instead, they form in clusters, and in these clustered environments newborn stars can have profound effects on one another and on their pa…