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[en] In addition to planetary perturbations, the small particles which make up a meteor stream are subject to outward radiation pressure and the Poynting-Robertson effect. New particles can also be generated in a stream through being released from the nucleus of a comet. The author summarises the main physical effects, discusses models for meteor stream evolution and gives a brief account of the observational data available. (Auth.)
Source
Markellos, V.V. (Patras Univ. (Greece)); Kozai, Y. (Tokyo Univ., Mitaka (Japan). Tokyo Astronomical Observatory) (eds.); Astrophysics and Space Science Library; v. 106; 424 p; ISBN 90-277-1650-1; 
; 1983; p. 83-87; D. Reidel; Dordrecht (Netherlands); 74. Colloquium of the International Astronomical Union on dynamical trapping and evolution in the solar system; Gerakini (Greece); 30 Aug - 2 Sep 1982
; 1983; p. 83-87; D. Reidel; Dordrecht (Netherlands); 74. Colloquium of the International Astronomical Union on dynamical trapping and evolution in the solar system; Gerakini (Greece); 30 Aug - 2 Sep 1982