@inproceedings{oai:jaxa.repo.nii.ac.jp:00003092,
 author = {Bell, Aaron C. and 尾中, 敬 and 土井, 靖生 and Galliano, Frederic and Wu, Ronin and 金田, 英宏 and 石原, 大助 and Giard, Martin and Bell, Aaron C. and Onaka, Takashi and Doi, Yasuo and Galliano, Frederic and Wu, Ronin and Kaneda, Hidehiro and Ishihara, Daisuke and Giard, Martin},
 book = {宇宙航空研究開発機構特別資料, JAXA Special Publication: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life},
 month = {Mar},
 note = {第4回「あかり」国際会議 (2017年10月17-20日. 東京大学), 文京区, 東京, The 4th AKARI International Conference: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life (October 17-20, 2017. The University of Tokyo), Bunkyo-ku, Tokyo, Japan, The anomalous microwave emission (AME) still lacks a conclusive explanation. This excess of emission, roughly between 10 and 50 GHz, correlates spatially with interstellar dust, prompting a 'spinning dust' hypothesis: electric dipole emission by rapidly rotating, small dust grains. The typical peak frequency range of the AME profile implicates grains on the order of 1 nm, suggesting polycyclic aromatic hydrocarbon molecules (PAHs). We compare AKARI/Infrared Camera (IRC), with its thorough PAH-band coverage, to AME intensity estimates from the Planck Collaboration, in the lambda Orionis region. We look also at infrared dust emission from other mid IR and far-IR bands. The results and discussion contained here apply to an angular scale of approximately 1 deg. In general, our results support an AME-from-dust hypothesis. In lambda Orionis, we find that certainly dust mass correlates with AME, and that PAH-related emission in the AKARI/IRC 9 micrometers band may correlate slightly more strongly., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730026018, レポート番号: JAXA-SP-17-009E},
 pages = {123--126},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {A look at possible microwave dust emission via AKARI infrared all-sky surveys},
 volume = {JAXA-SP-17-009E},
 year = {2018}
}