2015A&A...577A.115V

Most stars are born in clusters, thus the protoplanetary discs surrounding the newly formed stars might be influenced by this environment. Isolated star-disc encounters have previously been studied, and it was shown that very close encounters are necessary to completely destroy discs. However, relatively distant encounters are still able to change the disc size considerably. We quantify the importance of disc-size reduction that is due to stellar encounters in an entire stellar population. We modelled young, massive clusters of different densities using the code Nbody6 to determine the statistics of stellar encounter parameters. In a second step, we used these parameters to investigate the effect of the environments on the disc size. For this purpose, we performed a numerical experiment with an artificial initial disc size of 10⁵AU. We quantify to which degree the disc size is more sensitive to the cluster environment than to the disc mass or frequency. We show that in all investigated clusters a large portion of discs is significantly reduced in size. After 5Myr, the fraction of discs smaller than 1000AU in ONC-like clusters with an average number density of <ρ>_cluster∼60/pc³, the fraction of discs smaller than 1000AU is 65%, while discs smaller than 100AU make up 15%. These fractions increase to 84% and 39% for discs in denser clusters like IC 348 (<ρ>_cluster∼500/pc³). Even in clusters with a density four times lower than in the ONC (<ρ>_cluster∼15/pc³), about 43% of all discs are reduced to sizes below 1000 AU and roughly 9% to sizes below 100 AU. For any disc in the ONC that initially was larger than 1000 AU, the probability to be truncated to smaller disc sizes as a result of stellar encounters is quite high. Thus, among other effects, encounters are important in shaping discs and potentially forming planetary systems in stellar clusters.