We investigate the effects of the nearly fulfilled Efimov conditions on the properties of three-body resonances. Using the hyper-spheric adiabatic expansion method we compute energy distributions of fragments in a three-body decay of a nuclear resonance. As a realistic example we investigate the 1 − state in the halo nucleus 11 Li within a three-body 9 Li + n + n model. Characteristic features appear as sharp peaks in the energy distributions. Their origin, as in the Efimov effect, is in the large two-body s-wave scattering lengths between the pairs of fragments. Introduction. The Efimov effect was introduced more than thirty years ago as an anomaly in a three-body system arising when at least two of the three two-body swave scattering lengths approach infinity [1]. Then an increasing number of three-body bound states appear close to the two-body threshold even if there are no two-body bound states. The effect is prohibited by the Coulomb potential while only diminished by higher angular momentum [2]. Although entirely possible in molecules [3] the effect is unlikely to appear in nuclei due to unfavorable mass ratio [4,5].Still there exists a number of nuclear systems, called halos [3], which are natural three-body systems -a core plus two neutrons -where the Efimov condition of at least two large scattering lengths is nearly fulfilled. Although the unfortunate combination of the heavy core and light neutrons prohibits the appearance of bound Efimov states in the discrete spectrum, they still may appear as peculiar structures in the continuum. Very little, however, is known theoretically about the Efimov states in the continuum.