Characterization and dynamics of the peculiar stream Jhelum - A tentative role for the Sagittarius dwarf galaxy

Open Access

Fig. 13.

As Fig. 10, but now for initial conditions 4. Here in Panel (a) we see a more diffuse secondary component in the bottom, and a tertiary component in the top, see for comparison to Figs. 10–12. This stream also has a very clear separation of the components in v_rad, even fitting Jhelum1_5.

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