@inproceedings{oai:jaxa.repo.nii.ac.jp:00038387,
 author = {竹内, 拓 and 観山, 正見 and Takeuchi, Taku and Miyama, Shoken M.},
 book = {第28回月・惑星シンポジウム, Proceedings of the 28th ISAS Lunar and Planetary Symposium},
 month = {Dec},
 note = {Evolution of a protoplanetary disk under the tidal interaction between the disk and an embedded protoplanet is analyzed. The protoplanet excites density waves at its Lindblad resonances. As they propagate throughout the disk, these waves carry a flux of angular momentum which is eventually deposited into the gas at the locations where the waves are dissipated viscously. Protoplanets with a sufficiently large mass can induce the formation of a gap in the disk. The size of the gap and the structure of the disk are determined by the wave propagation length scale which is a decreasing function of viscosity. For small viscosity, density waves propagate to inner regions near the protostellar surface. Using an alpha prescription, we find that a Jupiter-mass protoplanet can lead to the removal of the inner disk if alpha is equal to or less than 3 x 10(exp -4)., 資料番号: AA0063352020},
 pages = {77--80},
 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 = {The evolution of the protoplanetary disks under the protoplanet's gravity},
 year = {1995}
}