Gamma Ray Bursts Session

Wednesday, 18 December 1996, 4:15-6:15 pm

Preliminary Program

Chairs: Ed Fenimore (LANL) and Kevin Hurley (Berkeley)

If you have any queries or comments on the program please email: Ed Fenimore, efenimore@lanl.gov or Kevin Hurley, khurley@sunspot.ssl.berkeley.edu



Speakers


4:15 Edison Liang (Rice University): Physical Model of Gamma-Ray Burst Spectral Evolution
4:35 Rob Preece (University of Alabama, Huntsville): Observations and Implications of X-Ray Excesses in GRBs
4:45 Tsvi Piran (Hebrew University): Physical Conditions in GRBs
5:05 Max Ruffert (Max-Planck Institute): Merging Neutron Stars as Central Engines for GRBs
5:15 K.S. Cheng (University of Hong Kong): Conversion of Neutron Stars to Strange Stars as a Possible Mechanism for GRBs
5:25 Hara Papathanassiou (Penn State): Spectral Properties of "Internal" and "External" Shock Models for GRBs
5:35 Nir Shaviv (Cal Tech) Gamma-Ray Bursts in Dense Stellar Environments - a Solution to the Riddle?
5:45 Ed Fenimore (Los Alamos National Lab): Expanding Relativistic Shells and Limitations on Temporal Variations in GRBs
5:55 Chuck Dermer (Naval Research Lab): Observational Implications of GRBs Occurring in Dense Stellar Clusters
6:05 Dieter Hartmann (Clemson University): What Does it Take to Solve the GRB Mystery?


Posters


Mechanisms:

Spectral:

Spatial Distributions:

Counterparts:

Instrumentation:

Miscellaneous: