@inproceedings{oai:jaxa.repo.nii.ac.jp:00020309,
 author = {Nouda, Akiyoshi and Emori, Hiroyuki and Nakazawa, Kiyoshi},
 book = {Proceedings of the 44th ISAS Lunar and Planetary Symposium},
 month = {},
 note = {44th  ISAS Lunar and Planetary Symposium (August 1-3,  2011. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)), Sagamihara, Kanagawa Japan, The collisions between protoplanets are occurred in the last stage of the planetary formation. Through these collisions, the Earth-Moon system was formed. Since, it is important to take the various configuration of collisional phenomena into consideration, when considering the origin of the Earth-Moon system. So, we investigate the parametric study of the collisions between the protoplanets. As a result, the redistribution of the mass is written in the simple form by using the remaining radius, in the region of the tidal disruption., 形態: カラー図版あり, 形態: CD-ROM1枚, Physical characteristics: Original contains color illustrations, Note: One CD-ROM, 資料番号: AA0065390024},
 publisher = {宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS), Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)},
 title = {Re-distribution of Mass and Angular Momentum through a Tidal Disruption between Protoplanets},
 volume = {44},
 year = {2011}
}