  This paper is concerned with the construction and analysis of boson stars in
the context of nonminimal derivative coupling theories. In particular we embed
our model in the biscalar extension of Horndeski gravity, considering a scalar
field theory displaying a nonminimally coupled kinetic term given by the
Einstein tensor. We focus on the case where the potential is given by a mass
term only, and when a six order self-interaction is included. In the latter
case we consider specific couplings in the self-interacting terms in such a way
that our self-interaction is given by a positive definite potential presenting
two degenerate local vacua. We show how solutions can be obtained and we
compare its principal properties with standard configurations constructed with
the usual minimally coupled kinetic term.
