  We study the gravitomagnetism in the TeVeS theory. We compute the
gravitomagnetic field that a slow-moving mass distribution produces in its
Newtonian regime. We report that the consistency between the TeVeS
gravitomagnetic field and that predicted by the Einstein-Hilbert theory leads
to a relation between the vector and scalar coupling constants of the theory.
We observe that requiring consistency between the near horizon geometry of a
black hole in TeVeS and the image of the black hole taken Event Horizon
Telescope leads to another relation between the coupling constants of the TeVeS
theory and enable us to identify the coupling constants of the theory.
