Notes. α, δ, V_g, q, e,a, ω, Ω, i and λ refer, respectively, to right ascension (°) and declination (°) of the radiant, geocentric velocity (km s⁻¹), perihelion distance (au), eccentricity, semi-major axis (°), argument of perihelion (°), longitude of the ascending node (°), inclination (°) and solar longitude (°) of the meteors orbits. “Dis” is the distance to the radiant. We kept displaying the D_sh criterion although we did not use it as a condition for associations. And over all, the criterion is less than 0.25. For few associations with asteroids orbits, which have a large semi-major axis a, it exceeds this value up to 1.5. The larger the semi-major axis of the orbits the larger the value of D_sh. For few associations with asteroids orbits, which have a large semi-major axis a, it exceeds this value up to 1.5. The larger the semi-major axis of the orbits the larger the value of D_sh. The same quantities are represented in Tables A.3–A.5.