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We investigate the kinematic evolution of planetesimals in self-gravitating discs, combining Smoothed Particle Hydrodynamical (SPH) simulations of the disc gas with a gravitationally coupled population of test particle planetesimals. We find that at
Externí odkaz:
http://arxiv.org/abs/1302.7216
Autor:
Walmswell, Joe1, Eldridge, John2
Publikováno v:
Proceedings of the International Astronomical Union. Apr2011 Supplement, Vol. 7 Issue S279, p419-420. 2p.
