  We investigate the radial perturbations of Ellis-Bronnikov wormholes
($\mathrm{l}=0$) in a slowly rotating background expanded up to second order in
rotation. We find indications that simple wormhole solutions such as
Ellis-Bronnikov in General Relativity can be stabilized by rotation, thus
favoring a viable traversable wormhole. This opens up the intriguing question
whether the many other wormhole solutions with or without the support of exotic
matter can become linearly mode stable when the wormhole rotates.
