Subir material

Suba sus trabajos a SEDICI, para mejorar notoriamente su visibilidad e impacto

 

Mostrar el registro sencillo del ítem

dc.date.accessioned 2020-03-26T10:44:06Z
dc.date.available 2020-03-26T10:44:06Z
dc.date.issued 1963
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/91811
dc.description.abstract A method for computing special perturbations has been devised. At the present time we have only considered the case with three co-planar bodies. Only one differential equation is to be solved. The radius vector r is the dependent variable. The time has been taken as independent variable. The true anomaly ν is the remaining quantity to be disturbed. The corresponding set of equations algebraic ones. The whole process is an iterative one. Special attention is to be paid for determining the most favorable cases for the applications. en
dc.format.extent 94-94 es
dc.language en es
dc.subject special perturbations es
dc.title Method for special perturbations en
dc.type Articulo es
sedici.creator.person Altavista, Carlos Alberto es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.event VI Reunión Científica de la Asociación Argentina de Astronomía (Horco Molle, Tucumán, 22 al 25 de mayo de 1963) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no. 6 es
dc.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/ es


Descargar archivos

Thumbnail
Resumen
Descargar archivo (52.50Kb) - PDF

Este ítem aparece en la(s) siguiente(s) colección(ones)

Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)