Evolutions of eccentricity and inclination for two asteroids that successfully crossed the resonance (two upper panels) and two asteroids that failed to cross the resonance (two lower panels). In each panel, two objects are distinguished by colours. The arrows in corresponding colour denote the moments of entering and leaving the resonance. All examples were randomly selected from the set of orbits Kor_in and the Yarkovsky drifting rate was ȧ_Y = 0.5 AU Gyr⁻¹.