@inproceedings{oai:jaxa.repo.nii.ac.jp:00005291,
 author = {深沢, 泰司 and 中澤, 知洋 and Fukazawa, Yasushi and Nakazawa, Kazuhiro},
 book = {宇宙航空研究開発機構特別資料, JAXA Special Publication: Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop},
 month = {Feb},
 note = {Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop (RIKEN, 10-12 June 2008), Hard X-ray emission from clusters of galaxies is important to probe the acceleration phenomena in the largest system in the universe. Here we presented Suzaku observations of A3376 and A3667. Upper limit of nonthermal hard X-ray emission gives a reasonable lower limit of intracluster magnetic field. Extremely hot gas component is found in A3667, indicating a suprathermal emission. We will suggest a possible hard X-ray mapping with MAXI to constrain the spatial distribution of hard X-ray emission., 資料番号: AA0064306052, レポート番号: JAXA-SP-08-014E},
 pages = {262--263},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Hard X-ray mapping of galaxy clusters},
 volume = {JAXA-SP-08-014E},
 year = {2009}
}