@inproceedings{oai:jaxa.repo.nii.ac.jp:00020716,
 author = {上辻, 勝也 and 鈴木, 仁志 and 木村, 勇気 and 齋藤, 嘉夫 and 墻内, 千尋 and Kamitsuji, Katsuya and Suzuki, Hitoshi and Kimura, Yuki and Saito, Yoshio and Kaito, Chihiro},
 book = {第36回月・惑星シンポジウム, Proceedings of the 36th ISAS Lunar and Planetary Symposium},
 month = {Nov},
 note = {Experimental studies of coalescence between MgO grains and SiO2 grains in smoke reveal the direct production of crystalline forsterite grains and amorphous Mg-bearing silicate owing to the difference of cooling velocity after the formation of Mg2SiO4 (forsterite) grains. This result suggests the observed crystalline Mg2SiO4 grains and amorphous Mg-bearing silicate in RSG, AGB, post-AGB and PNe were produced by the coalescence growth between MgO and SiO2 grains or Mg and SiO grains., 資料番号: AA0046650067},
 pages = {262--265},
 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 = {Crystalline forsterite grain formation due to the coalescence growth of MgO and SiO2 smoke particles},
 year = {2003}
}