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Fig. 3

image

Structure of the observable comet swarm triggered by Gliese 710. The initial parameters of the star are presented in the upper left corner while the parameters of the simulation are shown in the lower right one. The DLDW model (Dones et al. 1998) of the cloud was used. The projection of the GJ 710 heliocentric orbit is marked by a dashed line. The stellar perihelion (the position at the proximity) is shown as a big, black dot, while the small open circle denotes its anti-perihelion direction. The observable comet influx begins shortly after the star passage and gains its maximum 1 Myr later.

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