[M-GI36] Computational sciences on the universe, galaxies, stars, planets and their environments

[MGI36-P05] N-body simulations of planetary formation around M-dwarfs
considering planetesimal density differences

*Hiroaki Daido¹, Tenri Jinno¹, Takayuki Saitoh^1,2, Yoko Funato³, Yuki Yoshida², Junichiro Makino^1,2 (1. Department of Planetology, Graduate School of Science, Kobe University, Kobe, Japan, 2. Center for Planetary Science (CPS), Graduate School of Science, Kobe University, Kobe, Japan, 3. General Systems Studies, Graduate School of Arts and Sciences, The University of Tokyo, Tokyo, Japan)

Keywords:Planetary formation, N-body simulation, M-dwarf