When a star falls within a critical distance from a supermassive black hole, it is disrupted, and its debris are in part accreted by the black hole. The accretion in these Tidal Disruption Event (TDE) results in a flare, and, in extreme cases, it can generate a  relativistic hadronic jet, where high energy neutrinos could be produced. Recently, IceCube has detected a neutrino in spatial- and time-coincidence with tidal disruption event AT2019dsg. I present a phenomenological concordance scenario for this TDE, that includes a relativistic jet with efficient neutrino production. The model is based on the observed radiation spectra from AT2019dsg, and is consistent with numerical simulations of TDEs. This scenario offers an interpretation of the IceCube observation, and suggests that X-ray bright TDEs might be promising neutrino sources.