A new method of perturbation theory and its application to the satellite problem of celestial mechanics.
Arenstorf, Richard F.
Journal für die reine und angewandte Mathematik, Tome 222 (1966), p. 113-145 / Harvested from Göttinger Digitalisierungszentrum
Access to full text
Publié le : 1966-01-01
EUDML-ID : urn:eudml:doc:150718 
@article{GDZPPN002181606,
     title = {A new method of perturbation theory and its application to the satellite problem of celestial mechanics.},
     journal = {Journal f\"ur die reine und angewandte Mathematik},
     volume = {222},
     year = {1966},
     pages = {113-145},
     zbl = {0141.22802},
     url = {http://dml.mathdoc.fr/item/GDZPPN002181606}
}

Arenstorf, Richard F. A new method of perturbation theory and its application to the satellite problem of celestial mechanics.. Journal für die reine und angewandte Mathematik, Tome 222 (1966) pp. 113-145. http://gdmltest.u-ga.fr/item/GDZPPN002181606/