Significant age range in massive star cluster excluded by tight sub-giant-branch morphology
Supercomputing in High Energy Physics Horst Severini OU Supercomputing Symposium, September 12-13, 2002.
IMA, 11/19/04 Multiscale Modeling of Epitaxial Growth Processes: Level Sets and Atomistic Models Russel Caflisch 1, Mark Gyure 2, Bo Li 4, Stan Osher 1,
Chapter 5 Light: The Cosmic Messenger. 5.2 Learning from Light Our goals for learning What types of light spectra can we observe? How does light tell.
Microfluidic Free-Surface Flows: Simulation and Application
28 vi 2012Denver1 The Accelerating Universe Roger Blandford KIPAC Stanford.
Microfluidic Free-Surface Flows: Simulation and Application J.E Sprittles Y.D. Shikhmurzaev Indian Institute of Technology, Mumbai November 5 th 2011 The.
02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??
Dynamic Wetting Processes: Modelling and Simulation
Probing Out of E quilibrium Physics
PHENIX: The Next BUP and the Next Decade
The Accelerating Universe