Near-Infrared High-Resolution Spectroscopy of the Obscured AGN IRAS 01250+2832

• 白旗, 麻衣

• 臼田, 知史

• 大藪, 進喜

• 中川, 貴雄

• 山村, 一誠

• Shirahata, Mai

• Usuda, Tomonori

• Oyabu, Shinki

• Nakagawa, Takao

• Yamamura, Issei

Abstract

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

Journal

• 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

  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 JAXA-SP-17-010E 103-105, 2018-03-09

  宇宙航空研究開発機構(JAXA)

Details

• CRID: 1050011086257274240
• NII Article ID: 120006827229
• ISSN: 24332232
• Web Site: http://id.nii.ac.jp/1696/00002993/
• Text Lang: en
• Article Type: conference paper
• Data Source:
  • IRDB
  • CiNii Articles