Back to the Abstract

	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
	References

List of figures