In this paper, we study the charged and uncharged BTZ counterpart of the
    Black-Bounce proposed by Simpson and Visser recently. For the uncharged case,
    we find that the temperature is not modified by the bounce parameter. We also
    find that the wormhole side of the solution must always be supported by exotic
    matter over the throat. For the charged case we find that the thermodynamics is
    changed and the bounce parameter enlarges the region of stability. For both
    cases, we find that there are no stable orbits.

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