An approximate solution to the energy change of a circular binary in a parabolic three-body encounter
- Autor
- HUANG, T.-Y1 ; VALTONEN, M. J
[1] Univ. Nanjing, dep. astronomy, Nanjing, China - Fuente
Monthly Notices of the Royal Astronomical Society. 1987, Vol 229, Num 2, pp 333-344 ; ref : 11 ref
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Campo Científico
- Astronomy earth cosmic environment
- Editor
- Blackwell Science, Oxford
- País de la publicación
- United Kingdom
- Tipo de documento
- Article
- Idioma
- English
- Palabra clave (fr)
- Calcul numérique Espace phase Excentricité Fonction analytique Limite stabilité Problème 3 corps Théorie perturbation
- Palabra clave (in)
- Numerical calculation Phase space Eccentricity Analytical function Stability boundary Three body problem Perturbation theory
- Palabra clave (es)
- Cálculo numérico Espacio fase Excentricidad Función analítica Límite estabilidad Problema 3 cuerpos Teoría perturbación
- Clasificación
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03A Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations / 001E03A10 Fundamental astronomy
- Disciplina
- Astronomy
- Procedencia
- Inist-CNRS
- Base de datos
- PASCAL
- Identificador INIST
- 7685306
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1093/mnras/229.3.333 
https://dx.doi.org/10.1093/mnras/229.3.333
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