Abstract
The dynamical evolution of meteoroid streams associated with cornets Encke, Halley, Machholz 1986 VIII and asteroid Phaethon is discussed. It is shown that the planetary perturbations can greatly increase the streams thickness and each stream may produce several couples of meteor showers active in different seasons of the year. The theoretical and observed data are in a satisfactory accordance.
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Babadzhanov, P.B., Obrubov, Y.V. Evolution of short period meteoroid streams. Celestial Mech Dyn Astr 54, 111–127 (1992). https://doi.org/10.1007/BF00049547
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DOI: https://doi.org/10.1007/BF00049547