The Orbital Behavior at the Neighborhood of Stable Periodic Orbits in a 3D Galactic Potential

Details The Orbital Behavior at the Neighborhood of Stable Periodic Orbits in a 3D Galactic Potential The Orbital Behavior at the Neighborhood of Stable Periodic Orbits in a 3D Galactic Potential

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..424..380k&link_type=abstract

Proceedings of the 9th International Conference of the Hellenic Astronomical Society, proceedings of a conference held 20-24 Sep

Statistics

Applications

Scientific paper

In this paper we study the structure of invariant tori at the neighborhood of stable periodic orbits in a Hamiltonian system with three degrees of freedom of galactic type. The system we used for our applications rotates around its z-axis with angular velocity Ωb. The Potential of the system in Cartesian coordinates is:

Affiliated with

Also associated with

No associations

Rating

The Orbital Behavior at the Neighborhood of Stable Periodic Orbits in a 3D Galactic Potential does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Orbital Behavior at the Neighborhood of Stable Periodic Orbits in a 3D Galactic Potential, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Orbital Behavior at the Neighborhood of Stable Periodic Orbits in a 3D Galactic Potential will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-954100