Asteroidal-meteoric complexes.

Astronomy and Astrophysics – Astronomy

Scientific paper

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Minor Planets: Meteor Streams, Solar System: Families

Scientific paper

Fourteen asteroidal-meteoric complexes were identified by means of the criterion of similarity of quasistationary parameters μ, ν and Tisserand's invariant Ti. Each of these complexes consists of several meteor swarms and one or several asteroids. The existence of such complexes confirms the possibility of formation of meteor swarms by means of disintegration of asteroids and their fragments.

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