The following two pictures show the Kepler orbit of two masses $m_1, m_2$, where $m_1/m_2=7/3$, as I calculated them using $$ r(\varphi)=\frac{a(1-\varepsilon^2)}{1+\varepsilon\cos\varphi},\quad\boldsymbol{x}_1=\frac{m_2}{M} \boldsymbol{r},\quad\boldsymbol{x}_2=-\frac{m_1}{M} \boldsymbol{r} $$ with eccentricity $\varepsilon=0.825,1.25$ and $M=m_1+m_2$. In the pictures, $\times$ denotes the focus, $+$ the origin, that is the barycenter. The brown orbit belongs to $\boldsymbol{r}=\boldsymbol{x}_1-\boldsymbol{x}_2$, while pink belongs to $\boldsymbol{x}_1,\boldsymbol{x}_2$, respectively.
Now, the elliptic case is clear to me and looks as expected. But what about the hyperbolic case? How to explain the $>>$-shaped arcs ($<<$ respectively)? Before moving from one $>$-arc to the other $>$-arc, the object goes to infinity, so is that really the actual orbit or do I have an error in my simulation?