@inproceedings{oai:jaxa.repo.nii.ac.jp:00002999,
 author = {白旗, 麻衣 and 臼田, 知史 and 大藪, 進喜 and 中川, 貴雄 and 山村, 一誠 and Shirahata, Mai and Usuda, Tomonori and Oyabu, Shinki and Nakagawa, Takao and Yamamura, Issei},
 book = {宇宙航空研究開発機構特別資料, JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe},
 month = {Mar},
 note = {SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan, We provide a new physical insight on the hot molecular clouds near the nucleus of the heavily obscured AGN IRAS 01250+2832, based on the results of near-infrared high-resolution spectroscopy of gaseous CO ro-vibrational absorption lines with Subaru/IRCS+AO188. The detected CO absorption lines up to highly excited rotational levels reveal that hot dense molecular clouds exist around the AGN under the extreme physical conditions., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027022, レポート番号: JAXA-SP-17-010E},
 pages = {103--105},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Near-Infrared High-Resolution Spectroscopy of the Obscured AGN IRAS 01250+2832},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}