INVESTIGADORES
ORELLANA Rosa Beatriz
artículos
Título:
Orbit's Structure in the Isosceles Rectilinear Restricted Three-Body Problem
Autor/es:
J. MARTINEZ ALFARO AND R. B. ORELLANA
Revista:
CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY
Editorial:
SPRINGER
Referencias:
Lugar: Berlin; Año: 1997 vol. 67 p. 275 - 291
ISSN:
0923-2958
Resumen:
The isosceles rectilinear restricted three-body problem can be considered as the Sitnikov?s problem with eccentricity one or, as the isosceles problem when the central mass is zero and the primaries move having consecutive elliptic collisions. We compactify the phase space and analyze the flow on their boundary. This allows us to separate the phase space into different regions depending on the kind of orbits.
