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Results:
1-9
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Results: 9
Authors:
Kifonidis, K
Muller, E
Plewa, T
Citation: K. Kifonidis et al., Non-spherical core collapse supernovae and nucleosynthesis, NUCL PHYS A, 688(1-2), 2001, pp. 168C-171C
Authors:
Kritsuk, A
Plewa, T
Muller, E
Citation: A. Kritsuk et al., Convective cores in galactic cooling flows, M NOT R AST, 326(1), 2001, pp. 11-22
Authors:
Plewa, T
Muller, E
Citation: T. Plewa et E. Muller, AMRA: An Adaptive Mesh Refinement hydrodynamic code for astrophysics, COMP PHYS C, 138(2), 2001, pp. 101-127
Authors:
Kudlicki, A
Chodorowski, M
Plewa, T
Rozycka, M
Citation: A. Kudlicki et al., Reconstructing cosmic peculiar velocities from the mildly non-linear density field, M NOT R AST, 316(3), 2000, pp. 464-472
Authors:
Kifonidis, K
Plewa, T
Janka, HT
Muller, E
Citation: K. Kifonidis et al., Nucleosynthesis and clump formation in a core-collapse supernova, ASTROPHYS J, 531(2), 2000, pp. L123-L126
Authors:
Ciecielag, P
Plewa, T
Rozyczka, M
Citation: P. Ciecielag et al., High-resolution simulations and visualization of protoplanetary disks: structure of the flow in the vicinity of a massive planet, ASTRON NACH, 321(3), 2000, pp. 171-174
Authors:
Cox, DP
Shelton, RL
Maciejewski, W
Smith, RK
Plewa, T
Pawl, A
Rozyczka, M
Citation: Dp. Cox et al., Modeling W44 as a supernova remnant in a density gradient with a partiallyformed dense shell and thermal conduction in the hot interior. I. The analytical model, ASTROPHYS J, 524(1), 1999, pp. 179-191
Authors:
Shelton, RL
Cox, DP
Maciejewski, W
Smith, RK
Plewa, T
Pawl, A
Rozyczka, M
Citation: Rl. Shelton et al., Modeling W44 as a supernova remnant in a density gradient, with a partially formed dense shell and thermal conduction in the hot interior. II. The hydrodynamic models, ASTROPHYS J, 524(1), 1999, pp. 192-212
Authors:
Plewa, T
Muller, E
Citation: T. Plewa et E. Muller, The consistent multi-fluid advection method, ASTRON ASTR, 342(1), 1999, pp. 179-191
Risultati:
1-9
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