Gaps in stellar streams as a result of globular cluster flybys - The case of Palomar 5

Open Access

Table 1

Parameters determining the data volume.

N_p	N_ts	N_phase	N_sampling
100000	5000	6	50

Notes. N_p is the number of particles, N_ts is the number of time-steps saved, N_phase is the number of phase space coordinates, and N_sampling is the number of Monte-Carlo samplings of the initial conditions.

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