@inproceedings{oai:jaxa.repo.nii.ac.jp:00002998,
 author = {Wu, Ronin},
 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 present the spectral observation results from M83 and 30 Doradus, using the Spectral and Photometric Imaging REceiver (SPIRE) of the Herschel Space Observatory. The warm CO lines covered in this wavelength include J =4-3 to J =13-12 transitions, which allow us to determine the peak CO ladder intensities and beyond. We model the physical conditions in the objects (N(CO), T(sub kin), n(H2)) using a large velocity gradient (LVG) code. We also investigate the [N II] 205 μm map from M83 and compare our result with the CO J =1-0 and Hα maps., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027021, レポート番号: JAXA-SP-17-010E},
 pages = {99--101},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {The First Broad-Range CO Ladders from the M83 and 30 Doradus},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}