@inproceedings{oai:jaxa.repo.nii.ac.jp:00020505,
 author = {長沢, 真樹子 and 小久保, 英一郎 and Nagasawa, Makiko and Kokubo, Eiichiro},
 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 = {N-body simulation to investigate the growth of embryos in a close binary system is performed. Principal targets of the simulations are to investigate the possibility of the growth of the planets from the disk of planetesimals around Alpha Centauri. The inferred stable region around the close binary system is much smaller than the Solar system. The planetesimals orbit the host star with the modulating eccentricities, but their growth proceed almost the same way in the single star because of the effect of alignment of in periastrons., 資料番号: AA0063505043},
 pages = {166--169},
 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 = {Planetesimal growth in binary systems},
 year = {2006}
}