| dc.creator | Altavista, Carlos Alberto | |
| dc.date | 1970 | |
| dc.date | 2020-06-10T13:54:52Z | |
| dc.date.accessioned | 2023-07-14T20:46:07Z | |
| dc.date.available | 2023-07-14T20:46:07Z | |
| dc.identifier | http://sedici.unlp.edu.ar/handle/10915/97953 | |
| dc.identifier | issn:1669-9521 | |
| dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/7440523 | |
| dc.description | In Nº 13 of the Information Bulletin for the Southern Hemisphere I have given an outline of this method. Let there be thee mass points S = Sun, J = Jupiter, and A = Asteroid (or Satellite) and let us suppose that the orbital plane of Jupiter is taken as a fixed plane of reference in which a frame of fixed axes has been chosen in such a way that the X axis is oriented towards the perihelion of Jupiter. This system will be called “System I”. | |
| dc.description | Asociación Argentina de Astronomía | |
| dc.format | application/pdf | |
| dc.language | en | |
| dc.rights | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
| dc.rights | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
| dc.subject | Astronomía | |
| dc.subject | Galaxias | |
| dc.title | A new method for computing special perturbations in the three-body problem | |
| dc.type | Articulo | |
| dc.type | Comunicacion | |
