@inproceedings{oai:jaxa.repo.nii.ac.jp:00004955,
 author = {勝田, 哲 and Katsuda, Satoru},
 book = {宇宙航空研究開発機構特別資料:, JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H},
 month = {Feb},
 note = {The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan, The X-ray Imaging Spectrometer (XIS) onboard Suzaku is characterized by three major advantages: low and stable background, good response in low energies, and superior energy resolution. Utilizing these advantages, the XIS has attacked a number of supernova remnants (SNRs). The first advantageous point allows us to detect Fe, Mn, and Cr lines from young SNRs, while the second one reveals C and N lines from evolved SNRs. The third one enables us to detect line broadening due to either the Doppler effect, the thermal Doppler effect, or the ionization-timescale variation of several plasma components. For largely extended evolved SNRs, by combining the three advantages, spatially-resolved spectral analyses show us their metal distributions in unprecedented details. I will review such a Suzaku view of thermal SNRs, Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science, 資料番号: AA0064574023, レポート番号: JAXA-SP-09-008E},
 pages = {62--65},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Suzaku View of Thermal Supernova Remnants},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}