  We address the issue of whether a no-go theorem for static, spherically
symmetric wormholes, proven in Horndeski theories, can be circumvented by going
beyond Horndeski. We show that the ghost instabilities which are at the heart
of the no-go theorem, can indeed be avoided. The wormhole solutions with the
latter property are, however, strongly fine tuned, and hence it is likely that
they are unstable. Furthermore, it remains unclear whether these solutions have
other pathologies, like gradient instabilities along angular and radial
directions.
