Greg L. Bryan

Personal data

Education

1990-1996

Ph.D. in astronomy from the University of Illinois at Urbana-Champaign, Urbana, IL 61801.

1985-1989

BSc in physics from the Department of Physics, University of Calgary, Calgary, AB, Canada, T2N 1N4.

Awards and Honours

1997-present

Lyman Spitzer Fellowship, Department of Astrophysical Sciences, Princeton University

1990-1991

Departmental Fellowship, Department of Astronomy, University of Illinois at Urbana-Champaign

1985-1986

University of Calgary Scholarship, University of Calgary, Canada

Positions Held

1997-present

Lyman Spitzer Fellow, Princeton University Observatory.

1996-1997

Research Associate, Massachussets Institute of Technology.

1992-1996

Research Assistant, National Center for Supercomputing Applications.

1991-1992

Teaching Assistant, University of Illinois Astronomy Department.

1990-1991

Fellow, University of Illinois Astronomy Department.

1989-1990

Research Assistant, University of Colorado.

Refereed Publications

• Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons.
  Bryan, G.L., Norman, M.L., 1997, ApJ, in press.
  
  
• The X-Ray Luminosity Function and Gas Mass Function for Optically Selected Poor and Rich Clusters of Galaxies,
  Burns, J.O., Ledlow, M.J., Loken, C., Klypin, A., Voges, W., Bryan, G.L., Norman, M.L., White, R.A., 1996, ApJL 467, L49.
  
  
• A Piecewise Parabolic Method for Cosmological Hydrodynamics,
  Bryan, G.L., Norman, M.L., Stone, J.M., Cen, R., Ostriker, J.P., 1995, Computer Physics Communication 89, 149.
  
  
• A Parallel Self-consistent Field Code,
  Hernquist, L., Sigurdsson, S., Bryan, G.L., 1995, Astrophysical Journal, 446, 717.
  
  
• The Evolution of X-ray Clusters in a Cold Plus Hot Dark Matter Universe,
  Bryan, G.L., Klypin, A., Loken, C., Norman, M.L., Burns, J.O., 1994, Astrophysical Journal, 437, L5.
  
  
• A Comparison of Cosmological Hydrodynamic Codes,
  Kang, H., Ostriker, J.P., Cen, R., Ryu, D., Hernquist, L., Evrard, A.E., Bryan, G.L., Norman, M.L., 1994, Astrophysical Journal, 430, 83.
  
  
• X-ray Clusters from a High-Resolution Hydrodynamic PPM Simulation of the Cold Dark Matter Universe,
  Bryan, G.L., Cen, R., Norman, M.L., Ostriker, J.P., Stone, J.M., 1994, Astrophysical Journal, 428, 405.
  
  
• Energy Distributions of Symbiotic Novae,
  Bryan, G.L., Kwok, S., 1991, Astrophysical Journal, 368, 252.
  
  
• On the Formation of Carbon Stars,
  Bryan, G.L., Volk, K., Kwok, S., 1991, Astrophysical Journal, 365, 301.
  
  

Non-refereed Publications

• A Hybrid AMR Application for Cosmology and Astrophysics,
  Bryan, G.L., Norman, M.L., to appear in the "Workshop on Structured Adaptive Mesh Refinement Grid Methods", Mar. 1997, ed. N. Chrisochoides.
  
  
• Simulation X-ray Clusters with Adaptive Mesh Refinement,
  Bryan, G., Norman, M.L. in Proceedings of the 12th `Kingston meeting' on Theoretical Astrophysics: Computational Astrophysics (ASP Conference Series, 123), 1997, eds. D. A. Clarke & M. J. West, (San Francisco: ASP), p. 363.
  
  
• The Numerical Simulation of X-ray Clusters
  Bryan, G. 1996, Ph.D. Thesis, University of Illinois at Urbana-Champaign.
  
  
• High-Resolution 3D Simulations and Jet Turbulence,
  Loken, C., Burns, K., Bryan, G., Norman, M. 1996, to appear in Energy Transport in Radio Galaxies and Quasars, ASP Conference Series, eds. P. Hardee, A. Bridle, and A. Zensus.
  
  
• A Hydrodynamic Simulation of Cluster Formation,
  Bryan, G.L., Norman, M.L., 1994, in Numerical Simulations in Astrophysics, eds. Franco, J., Lizano, S., Aguilar, L., Daltabuit, E. (Cambridge: Cambridge University Press), 73.
  
  
• Adapting CMHOG to Cosmological Studies,
  Bryan, G.L., 1992, NCSA Technical Report 004.