@inproceedings{oai:jaxa.repo.nii.ac.jp:00020502,
 author = {高橋, 啓介 and 小林, 浩 and 渡邊, 誠一郎 and Takahashi, Keisuke and Kobayashi, Hiroshi and Watanabe, Seiichiro},
 book = {第39回月・惑星シンポジウム, Proceedings of the 39th ISAS Lunar and Planetary Symposium},
 month = {Aug},
 note = {Solar system has experienced planetary migration in its formation stage. Especially, Neptune has an evidence of outward migration in the 3:2 mean motion resonance in the Kuiper belt objects. In the point of view of planetary formation theory, outer ice giant planet needs planetary migration to shortening its growth time. Several simulations about planetary migration has done, and some results indicate that planet can migrate outward when disk has enough mass, but there are few works to understand the basic mechanism. In our work, we would like to focus attention on the mass flux that step over the planet to formulate the planetary migration. That kind of mass flux works as a fuel of migration., 資料番号: AA0063505040},
 pages = {154--157},
 publisher = {宇宙航空研究開発機構宇宙科学研究本部, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS)},
 title = {Formulation of planetary migration},
 year = {2006}
}