@inproceedings{oai:jaxa.repo.nii.ac.jp:00005032,
 author = {広津, 敏尚 and 堂谷, 忠靖 and 尾崎, 正伸 and 馬場, 彩 and 穴田, 貴康 and Hirotsu, Toshihisa and Dotani, Tadayasu and Ozaki, Masanobu and Bamba, Aya and Anada, Takayasu and Balucinska-Church, M. and Church, M. J.},
 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, We report Suzaku observation of the dipping, bursting low-mass X-ray binary XB 1323-619 focusing on the iron absorption lines in the energy spectra. The source was found to be dim, 1.5 x 10(exp 36) ergs/s (1-10 keV, 10 kpc), during the Suzaku observation in 2007 contrary to the brightening trend continued between 1985 and 2003. Clear absorption lines of He/H-like iron ions were detected in the persistent and dip spectra of the Suzaku data. In spite of the luminosity difference of a factor of 4, the equivalent widths (EWs) of the absorption lines and their changes in the dip were not very different from those observed by XMM-Newton in 2003. We considered the cause of similarity in EWs in the framework of the standard disk model., 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: AA0064574100, レポート番号: JAXA-SP-09-008E},
 pages = {274--275},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Suzaku Observation of the Iron Absorption Lines in the Dipping Low-Mass X-ray Binary XB1323-619},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}