In the absence of a non-axisymmetric perturbation, the orbits
can be computed in the epicyclic approximation, and the variables
,
<< r0 follow the evolution of an harmonic
oscillator, with the epicyclic frequency
.
In the presence
of a bar perturbation, the equations of motions, in the
reference frame rotating with the perturbation at
are
(Lindblad & Lindblad 1994):
The oscillator is now forced by an external perturbation at the
imposed frequency
.
Taking for
and
a solution of the form:
Acknowledgements
We wish to thank Jean-Gabriel Cuby and Claire Moutou for their help and support during the ISAAC observations. We also wish to thank the referee, Alan Morwood, for a detailed and critical reading of the manuscript. This work has been supported by the Swiss National Science Foundation.
Copyright ESO 2001