@inproceedings{oai:jaxa.repo.nii.ac.jp:00004951,
 author = {Takata, Jumpei and Taam, Ronald E.},
 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 spectral energy distribution from the X-ray to the very high energy regime (> 100 GeV) has been investigated for the gamma-ray binary system PSR B1259-63/SS2883 as a function of orbital phase within the framework of a simple model of a pulsar wind nebula. The emission model is based on the synchrotron radiation process for the X-ray regime and the inverse Compton scattering process boosting stellar photons from the Be star companion to the very high energy (100GeV-TeV) regime. With this model, the observed temporal behavior can, in principle, be used to probe the pulsar wind properties at the shock as a function of the orbital phase., 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: AA0064574019, レポート番号: JAXA-SP-09-008E},
 pages = {50--51},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Probing the Pulsar Wind in the gamma-ray Binary System: PSR B1259-63/SS 2883},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}