Back to the Abstract

Article Contents
1 Introduction
2 The nature of galactic perturbations
3 Observable comets produced by the Galactic disk tide alone
4 Mixing stellar and galactic perturbations
5 Dynamical filtering
6 Monte Carlo simulation scheme
7 General stellar effect on the cloud
8 Perihelion direction distribution of simulated observable comets and the time-dependence of their influx
9 Conclusions

List of figures

Copyright ESO 2005
Published by EDP Sciences