×

zbMATH — the first resource for mathematics

Secular perturbations of resonant asteroids. (English) Zbl 0577.70014

MSC:
70F15 Celestial mechanics
PDF BibTeX XML Cite
Full Text: DOI
References:
[1] Giacaglia, G.E.O.: 1968,Smithsonian Astrophysical Observatory, Special Report, No. 278.
[2] Giacaglia, G.E.O.: 1969,Astron. J. 74, 1254. · doi:10.1086/110930
[3] Giacaglia, G.E.O. and Nacozy, P.E.: 1970, in G.E.O. Giacaglia (ed.),Periodic Orbits, Stability and Resonances, 96?127, D. Reidel Publ. Co., Dordrecht. · Zbl 0263.70009
[4] Hori, G. and Giacaglia, G.E.O.: 1968,Research in Celestial Mechanics and Differential Equations, University of Sao Paulo, 67-68-01.
[5] Kinoshita, H. and Nakai, H.: 1983,private communication.
[6] Kozai, Y.: 1962,Astron. J. 67, 5891?598.
[7] Kozai, Y.: 1979, in R.L. Duncombe (ed.),Dynamics of the Solar System, D. Reidel Publ. Co., Dordrecht, 231?237.
[8] Kozai, Y.: 1980,Icarus 41, 89?95. · doi:10.1016/0019-1035(80)90161-X
[9] Nacozy, P.E. and Diehl, R.E.: 1974,Celest. Mech. 8, 445. · doi:10.1007/BF01227797
[10] Nacozy, P.E. and Diehl, R.E.: 1978a.Astron. J. 83, 522. · doi:10.1086/112231
[11] Nacozy, P.E. and Diehl, R.E.: 1978b,Celest. Mech. 17, 405. · doi:10.1007/BF01228960
This reference list is based on information provided by the publisher or from digital mathematics libraries. Its items are heuristically matched to zbMATH identifiers and may contain data conversion errors. It attempts to reflect the references listed in the original paper as accurately as possible without claiming the completeness or perfect precision of the matching.