Abstract
We consider the three-dimensional bounded motion of a test particle around razor-thin disk configurations, by focusing on the adiabatic invariance of the vertical action associated with disk-crossing orbits. We find that it leads to an approximate third integral of motion predicting envelopes of the form \(Z(R)\propto [\varSigma (R)]^{-1/3}\), where R is the radial galactocentric coordinate, Z is the z-amplitude (vertical amplitude) of the orbit and \(\varSigma \) represents the surface mass density of the thin disk. This third integral, which was previously formulated for the case of flattened 3D configurations, is tested for a variety of trajectories in different thin-disk models.
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Notes
Here, the term “small” means small enough to neglect variations in the projection of the orbit on the \(z=0\) plane.
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Acknowledgments
The work of R.S.S.V. is supported by the “São Paulo Research Foundation” (FAPESP), grants 2010/00487-9 and 2015/10577-9. RSSV thanks Alberto Saa for fruitful discussions and Sylvio Ferraz Mello for helpful remarks on the accepted version of the manuscript. The authors thank the anonymous referees for insightful comments which helped us improve the final version of the manuscript. The authors also acknowledge the support from FAPESP grant 2013/09357-9.
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Vieira, R.S.S., Ramos-Caro, J. Integrability of motion around galactic razor-thin disks. Celest Mech Dyn Astr 126, 483–500 (2016). https://doi.org/10.1007/s10569-016-9705-0
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DOI: https://doi.org/10.1007/s10569-016-9705-0