Asymmetry in the tidal tails of open star clusters from direct N-body integrations in Milgrom-law dynamics

Open Access

Fig. 4

Centre of mass motions. The straight blue lines refer to the MLD-centre of mass (Eq. (46)) whereas the wobbling red curves show the Newtonian centre of mass, $R_{com, New} = \frac{m_{1} q_{1} + m_{2} q_{2}}{m_{1} + m_{2}}$ ${{\bf{R}}_{{\rm{com}},{\rm{New}}}} = {{{m_1}{{\bf{q}}_1} + {m_2}{{\bf{q}}_2}} \over {{m_1} + {m_2}}}$ . The x-component of both centers of mass runs horizontally, the y-component increases continuously.

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