On the homogeneous form of the differential equations of relative motion of the three-body problem

Autores
Altavista, Carlos Alberto
Año de publicación
1982
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
It has previously been shown (Celestial Mechanics, Vol. 6 Nº 2, September 1972) that the system of differential equations of relative motion of the three-body problem can br brought into a homogeneous form. We give here an account of some additional proofs concerning the conditions of convergence of the geometric process used to obtain the new equations as well as a theorem due to Kolmogorov to consider analytical aspects of the problem.
Asociación Argentina de Astronomía
Materia
Astronomía
Galaxias
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/111812
Acceder
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repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling On the homogeneous form of the differential equations of relative motion of the three-body problemAltavista, Carlos AlbertoAstronomíaGalaxiasIt has previously been shown (Celestial Mechanics, Vol. 6 Nº 2, September 1972) that the system of differential equations of relative motion of the three-body problem can br brought into a homogeneous form. We give here an account of some additional proofs concerning the conditions of convergence of the geometric process used to obtain the new equations as well as a theorem due to Kolmogorov to consider analytical aspects of the problem.Asociación Argentina de Astronomía1982info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf235-240http://sedici.unlp.edu.ar/handle/10915/111812enginfo:eu-repo/semantics/altIdentifier/issn/1669-9521info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T17:06:40Zoai:sedici.unlp.edu.ar:10915/111812Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:06:40.531SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv On the homogeneous form of the differential equations of relative motion of the three-body problem
title On the homogeneous form of the differential equations of relative motion of the three-body problem
spellingShingle On the homogeneous form of the differential equations of relative motion of the three-body problem
Altavista, Carlos Alberto
Astronomía
Galaxias
title_short On the homogeneous form of the differential equations of relative motion of the three-body problem
title_full On the homogeneous form of the differential equations of relative motion of the three-body problem
title_fullStr On the homogeneous form of the differential equations of relative motion of the three-body problem
title_full_unstemmed On the homogeneous form of the differential equations of relative motion of the three-body problem
title_sort On the homogeneous form of the differential equations of relative motion of the three-body problem
dc.creator.none.fl_str_mv Altavista, Carlos Alberto
author Altavista, Carlos Alberto
author_facet Altavista, Carlos Alberto
author_role author
dc.subject.none.fl_str_mv Astronomía
Galaxias
topic Astronomía
Galaxias
dc.description.none.fl_txt_mv It has previously been shown (Celestial Mechanics, Vol. 6 Nº 2, September 1972) that the system of differential equations of relative motion of the three-body problem can br brought into a homogeneous form. We give here an account of some additional proofs concerning the conditions of convergence of the geometric process used to obtain the new equations as well as a theorem due to Kolmogorov to consider analytical aspects of the problem.
Asociación Argentina de Astronomía
description It has previously been shown (Celestial Mechanics, Vol. 6 Nº 2, September 1972) that the system of differential equations of relative motion of the three-body problem can br brought into a homogeneous form. We give here an account of some additional proofs concerning the conditions of convergence of the geometric process used to obtain the new equations as well as a theorem due to Kolmogorov to consider analytical aspects of the problem.
publishDate 1982
dc.date.none.fl_str_mv 1982
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/111812
url http://sedici.unlp.edu.ar/handle/10915/111812
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/1669-9521
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
235-240
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instname:Universidad Nacional de La Plata
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reponame_str SEDICI (UNLP)
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instname_str Universidad Nacional de La Plata
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repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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