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BIBLIOGRAFIA



  1. (*) Bailey M.E., 1983, The structure and evolution of the Solar System comet cloud, Month. Notic. of R.A.S., vol.204, str.603.
  2. (*) Bailey M.E., 1986, The mean energy transfer rate to comets in Oort cloud and implications for cometary origin, Month. Notic. of R.A.S., vol.218, str. 1.
  3. Dormand J.R. i Prince P.J., 1978, New Runge-Kutta algorithms for numerical simulation in dynamical astronomy, Cel.Mech., vol.18, str.223.
  4. Everhart E., 1985, An efficient integrator that uses Gauss-Radau spacings, w "Dynamics of Comets, their Origin and Evolution", red. A.Carusi i G.B.Valsechi, D.Reidel Publ.Co.,str.185. Abstract
  5. (*) Fernandez J.A., 1980, On the existence of a comet belt beyond Neptune, Month. Notic. of R.A.S., vol.192, str. 481-491.
  6. Fernandez J.A., 1981, New and evolved comets in the Solar System, Astron. and Astrophys., vol. 96, str. 26.
  7. (*) Fernandez J.A., 1987, Time dependent injection of Oort cloud comets into Earth-crossing orbits, Icarus, vol.71, str.46. Abstract
  8. Fox K., 1984, Numerical integration of the equations of motion of celestial mechanics, Cel.Mech., vol.33, str. 127.
  9. (*) Froeschle C. i Rickman H., 1988, Monte Carlo modeling of cometary dynamics, Cel.Mech., vol.43, str. 265.
  10. Mignard F., i Remy F., 1985, Dynamical evolution of the Oort cloud. II: A theoretical approach, Icarus, vol.63, str. 20. Abstract
  11. Morris D.E. i O'Neill T.G., 1988, Limits on closest encounter with other star since formation of our Solar System, Astron. J., vol.96, numer 3, str. 1127.
  12. Odell A.W., Gooding R.H., 1986, The hyperbolic Kepler Equation ( and the Elliptic Equation revisited ), Cel. Mech., vol. 44, str. 267.
  13. Oort J.H.,1950,The structure of the cloud of comets surrounding the Solar System and a hypothesis concerning its origin,Bulletin of the Astronomical Institutes of the Netherlands, vol.XI,numer 408, str. 91.
  14. Öpik E., 1932,Note on stellar perturbations of nearly parabolic orbits, Proceedings of the American Academy of Arts and Sciences, vol.67, numer 6, str. 169.
  15. Remy F. i Mignard F., 1985, Dynamical evolution of the Oort cloud. I : A Monte Carlo simulation, Icarus, vol.63, str.1. Abstract
  16. Rickman H., 1976, Stellar perturbations of orbits of long-period comets and their significance for cometary capture, Bulletin of the Astronomical institutes of Czechoslovakia , vol. 27, numer 2, str. 92.
  17. (*) Rickman H. i Froeschle C., 1988, Cometary dynamics, Cel. Mech., vol.43, str. 243.
  18. Scholl H., Cazenave A., Brachic A., 1982, The effect of star passages on cometary orbits in the Oort cloud, Astron. and Astrophys., vol.112, srt. 157.
  19. Sekanina Z., 1968, On the perturbations of comets by near-by stars.II.Encounters of comets with fast moving stars, Bulletin of the Astronomical Institutes of Czechoslovakia, vol. 19 , str.291.
  20. Staniucha M.S. i Banaszkiewicz M., 1988, Passage of the Sun through an interstellar nebula and the Oort cloud comets, w "Few body problem",red. M.J. Valtonen,Kluwer Academic Press, str.201. Abstract
  21. Weissman P.R., 1980,Stellar perturbation on the cometary cloud, Nature, vol.288, str. 242. Abstract
  22. (*) Weissman P.R., 1982, Dynamical history of the Oort cloud, w "Comets", red. L.L.Wilkening, Univ.Arizona Press, Tuckson, str.637. Abstract
  23. (*) Weissman P.R., 1983, Dynamical evolution of the Oort cometary cloud, Highlights of Astronomy, vol.6, str.363. Abstract
  24. Weissman P.R.,1986, The Oort cloud in transition, w "Asteroids, Comets and Meteors II", red. A. Carusi i G.B.Valsechi, Uppsala Univ. Press, Uppsala, str.197.
  25. Yabushita S., 1972, Stellar perturbations of orbits of long period comets, Astron. and Astrophys., vol. 16, str. 395.
  26. Yabushita S., Hasegawa I., Kobayashi K., 1982,The stellar perturbations of orbital elements of long-period comets,Mon.Notic. of R.A.S., vol. 200, str. 661.
  27. (*) Yabushita, S., 1983, Processes of dynamical evolution of cometary orbits, Quarterly Journal of R.A.S., vol.24, str.430.

(*)Gwiazdką oznaczono publikacje przeglądowe, z których nie wszystkie cytowane są w tekście pracy.



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