Fluid trajectories from merger simulations

In the following, the ejecta properties of both compact object mergers and collisions are provided for scientific post-processing in nucleosynthesis calculations.

If you make use of the provided data, please make sure to read and cite the following papers:

• The multi-messenger picture of compact object encounters: binary mergers vs dynamical collisions
  S. Rosswog, T. Piran and E. Nakar,
  MNRAS 430 (4), pp.2585-2604 (2013)
• The Electromagnetic Signals of Compact Binary Mergers
  T. Piran, E. Nakar and S. Rosswog,
  MNRAS 430 (3), pp.2121-2136 (2013)
• On the astrophysical robustness of neutron star merger r-process
  O. Korobkin, S. Rosswog, A. Arcones and C. Winteler
  MNRAS 426, 1940 (2012)

Double neutron star mergers:

Neutron star - black hole mergers: