@inproceedings{oai:jaxa.repo.nii.ac.jp:00004952,
 author = {岸下, 徹一 and 高橋, 忠幸 and 田中, 孝明 and 内山, 泰伸 and 山岡, 和貴 and Kishishita, Tetsuichi and Takahashi, Tadayuki and Tanaka, Takaaki and Uchiyama, Yasunobu and Yamaoka, Kazutaka and Dmitry, Khangulyan and Aharonian, Felix A. and Bosch-Ramon, Valenti and Hinton, Jim A.},
 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 on the results from Suzaku and previous X-ray observations on the galactic binary LS5039, a TeV gamma-ray emitting binary. The Suzaku observation which covered continuously more than one orbital period revealed strong X-ray flux modulation at the orbital period for the first time, with its close resemblance to the TeV gamma-ray light curve. The X-ray data up to 70keV measured with Suzaku are described by a hard power-law spectrum with a phase-dependent photon index which varies within GAMMA = 1.45 - 1.6. We also found that the modulation curves are surprisingly stable in 1999 - 2007. The long-term behavior of the non-thermal X-ray light curves over eight years favors that a scenario in which the radiation is related to an ultrarelativistic pulsar wind would be able to account for the stable clock-like X-ray/TeV gamma-ray behaviors., 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: AA0064574020, レポート番号: JAXA-SP-09-008E},
 pages = {52--53},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Study of the Spectral and Temporal Characteristics of X-ray Emission of the Gamma-ray Binary LS 5039 with Suzaku},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}