Predicted favorable visibility conditions for anomalous tails of comets

  • Zdenek Sekanina
Cometary Dust
Part of the Lecture Notes in Physics book series (LNP, volume 48)


Meteor Stream Perihelion Distance Revolution Period Cometary Orbit Parent Comet 


Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.


  1. Cook, A. F. (1973), in “Evolutionary and Physical Properties of Meteoroids”, Hemenway, C. L., Millman, P. M., and Cook, A. F., Eds., NASA SP319, Washington, D.C., p. 183.Google Scholar
  2. Everhart, E., and Raghavan, N. (1970), Astron. J. 75, 258.Google Scholar
  3. Marsden, B. G. (1975), Catalogue of Cometary Orbits. (2nd edition.) IAU Central Bureau for Astronomical Telegrams, Smithsonian Astrophys. Obs.Google Scholar
  4. Roemer, E., and Lloyd, R. E. (1966), Astron. J. 71, 443.Google Scholar
  5. Sekanina, Z. (1973), Astrophys. Lett. 14, 175.Google Scholar
  6. Sekanina, Z. (1974), Sky and Tel. 47, 374.Google Scholar
  7. Sekanina, Z. (1975), Icarus 25, 218.Google Scholar
  8. Vsekhsvyatsky, S. K. (1958), Physical Characteristics of Comets. (In Russian.) Moscow, p. 51. (English transl.: Jerusalem, 1964.) Follow-ups: Soviet Astron. 6, 849 (1963); 10, 1034 (1967); and 15, 310 (1971).Google Scholar

Copyright information

© Springer-Verlag 1976

Authors and Affiliations

  • Zdenek Sekanina
    • 1
  1. 1.Center for Astrophysics Harvard College Observatory and Smithsonian Astrophysical ObservatoryCambridgeUSA

Personalised recommendations