@inproceedings{oai:jaxa.repo.nii.ac.jp:00004979,
 author = {山内, 茂雄 and Yamauchi, Shigeo},
 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, Suzaku observed the supernova remnant G344.7-0.1. An extended X-ray emission with a diameter of 6 min - 8 min was clearly found. In addition to emission lines from highly ionized Si, S, Ar, and Ca, the Xray spectrum exhibited a strong emission line at an energy of 6.465 keV from low-ionized Fe. The Fe K-line was represented by a broad Gaussian line model. The overall spectra in the 1-10 keV band were well represented by a two-component non-equilibrium ionization model. The results of a spectral fitting indicate that Si, S, Ca, and Fe are overabundant relative to the solar values., 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: AA0064574047, レポート番号: JAXA-SP-09-008E},
 pages = {122--123},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Suzaku Observation of the Supernova Remnant G344.7-0.1},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}