@inproceedings{oai:jaxa.repo.nii.ac.jp:00003138,
 author = {高橋, 英則 and 中西, 康一郎 and 松尾, 宏 and Takahashi, Hidenori and Nakanishi, Koichiro and Matsuo, Hiroshi},
 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, NGC 253 is well known local starburst galaxy which is currently undergoing a period of intense star formation. We present spatially resolved star-forming activity analysis of NGC 253 using multi-wavelength data from optical to radio. NGC 253 star-forming regions, especially those in the galactic center, are enshrouded by not a few amount of dust produced by their active star-formation. Star-formation tracers which suffer less dust extinction will be essential to investigate the star formation. Pa alpha emission line at 1.875 micrometers traces actual star-formation activity even at high extinction region that is difficult to measure it in optical wavelengths. We have carried out Pa narrow-band imaging observations which cannot be derived from ground based facilities except for TAO site. Low frequency (e.g. 1.4 GHz) radio continuum data taken with VLA and FIR forbidden lines with AKARI FIS/FTS and Herschel are also good tracers for current star-formation. Using above data and AKARI archive data the differences of star-formation activities among galactic center, bar, bar-end and inter-arm can be revealed., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730026064, レポート番号: JAXA-SP-17-009E},
 pages = {329--332},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Spatially Resolved Star-formation Activity of Starburst Galaxy NGC 253},
 volume = {JAXA-SP-17-009E},
 year = {2018}
}