Attachment A2
Publications Resulting from NPACI Research

  1. Tohline, J.E. and Cazes, J.E. 1997, "Early Experiences with the Cray T3E at the SDSC," a Technical Report submitted to the SDSC in June, 1997. (See online document "http:// faculty/ tohline/SDSC/ T3E.timings.html".)

  2. Tohline, J.E., Cazes, J.E., and Cohl, H.S. 1999, "The Formation of Common-Envelope, Pre-Main-Sequence Binary Stars," in Proceedings of Numerical Astrophysics 1998 [Tokyo, Japan], eds., S.M. Miyama, K.Tomishak, and T. Hanawa, p. 155. (See online document "http:// astro/ nap98/".)

  3. Cazes, J.E., Tohline, J.E., Cohl, H.S., and Motl, P.M. 1999, "A Heterogeneous Computing Environment to Simulate Astrophysical Fluid Flows," in Proceedings of the DoD Users' Group Conference, Monterey, CA. (See online document "http:// astro/ cazes/ dodconf/ hce.html".)

  4. Cohl, H.S. and Tohline, J.E. 1999, "A Compact Cylindrical Green's Function Expansion for the Solution of Potential Problems," The Astrophysical Journal, 527, 86.

  5. Cohl, H.S. 1999, "On the Numerical Solution of the Cylindrical Poisson Equation for Isolated Self-Gravitating Systems," Ph.D. Dissertation, Louisiana State University.

  6. Cazes, J.E. 1999, "The Formation of Short Period Binary Star Systems from Stable, Self-Gravitating Gaseous Bars," Ph.D. Dissertation, Louisiana State University.

  7. Cazes, J.E. and Tohline, J.E. 2000, "Self-Gravitating Gaseous Bars. I. Compressible Analogs of Riemann Ellipsoids with Supersonic Internal Flows," The Astrophysical Journal, 532, 1051.

  8. New, K.C.B., Centrella, J.M., and Tohline, J.E. 2000, "Gravitational Waves from Long-Duration Simulations of the Dynamical Bar Instability," Physical Review D, 62, 064019.

  9. Cohl, H.S., Tohline, J.E., Rau, A.R.P., and Srivastava, H.M. 2000, "Developments in Determining the Gravitational Potential using Toroidal Functions," Astronomische Nachrichten, 321, 1.

  10. Lindblom, L., Tohline, J.E. and Vallisneri, M. 2001, "Non-Linear Evolution of the r-Modes in Neutron Stars," Physical Review Letters, 86, 1152.

  11. Barnes, E.I. and Tohline, J.E. 2001, "Populating Stellar Orbits Inside a Rotating, Gaseous Bar," The Astrophysical Journal, 551, 80.

  12. Barnes, E.I. 2001, "A Study of Stellar Orbits in a Rotating, Gaseous Bar," Ph.D. Dissertation, Louisiana State University.

  13. Tohline, J.E. and Durisen, R.H. 2000, "An Update on Binary Formation by Rotational Fission," in Formation of Binary Stars (Proceedings of IAU 2000), eds. H. Zinnecker and R.D.Mathieu.

  14. Motl, P., Tohline, J.E. and Frank, J. 2002, "Numerical Methods for the Simulation of Dynamical Mass Transfer in Binaries," The Astrophysical Journal Supplement, 138, 121.

  15. Cohl, H.S., Rau, A.R.P., Tohline, J.E., Browne, D.A., Cazes, J.E., and Barnes, E.I. 2001, "Useful Alternative to the Multipole Expansion of 1/r Potentials," Physical Review A, 65, 052509.

  16. Lindblom, L., Tohline, J.E. and Vallisneri, M. 2002, "Numerical Evolutions of the r-Modes in Neutron Stars," Physical Review D, 65, 084039.