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