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We report measurements from an XMM-Newton observation of the low-excitationradio galaxy 3C 386. The study focusses on an X-ray-emitting gas belt, whichlies between and orthogonal to the radio lobes of 3C 386 and has a meantemperature of $0.94\pm0.05$ keV, cooler than the extended group atmosphere.The gas in the belt shows temperature structure with material closer to thesurrounding medium being hotter than gas closer to the host galaxy. We suggestthat this gas belt involves a `buoyancy-driven inflow' of part of the group-gasatmosphere where the buoyant rise of the radio lobes through the ambient mediumhas directed an inflow towards the relic cold core of the group.Inverse-Compton emission from the radio lobes is detected at a level consistentwith a slight suppression of the magnetic field below the equipartition value.

Buoyancy-driven inflow to a relic cold core: the gas belt in radio galaxy 3C 386