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A&A 372, 784-792 (2001)
DOI: 10.1051/0004-6361:20010571
Periodic orbits in warped disks
Y. Revaz and D. PfennigerGeneva Observatory, University of Geneva, 1290 Sauverny, Switzerland
(Received 22 November 2000 / Accepted 9 April 2001 )
Abstract
It is often assumed that a warped
galaxy can be modeled by a set of rings.
This paper verifies numerically
the validity of this assumption by the study of periodic orbits populating a
heavy self-gravitating warped disk.
The phase space structure of a warped model reveals that the circular periodic
orbits of a flat disk are transformed in quasi annular periodic orbits which conserve their stability. This lets us also explore
the problem
of the persistence of a large outer warp. In particular,
the consistency of its orbits with the density distribution is checked as a
function of the pattern speed.
Key words: galaxies: kinematics and dynamics of galaxies -- galaxies: spiral
Offprint request: Y. Revaz, Yves.Revaz@obs.unige.ch
© ESO 2001
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