@article{oai:teapot.lib.ocha.ac.jp:00034607,
 author = {Orito, Erimi and Kawamura, Tetuya},
 issue = {1},
 journal = {お茶の水女子大學自然科學報告},
 month = {Aug},
 note = {application/pdf, 紀要論文, Smoothed Particle Hydrodynamics (SPH) simulation is carried out to find the possibility of spiral shock wave in accretion disk in primitive planetary system. In order to avoid uncertainness due to artificial viscous term, we employ SPH method combined with Riemann solver in this study. We have shown that the spiral shock wave can be formed in primitive planetary system under the limiting initial conditions of temperature and angular velocity.},
 pages = {1--8},
 title = {Generation of spiral shock wave in the simulation of formation of accretion disk in primitive planetary system},
 volume = {59},
 year = {2008}
}