@inproceedings{oai:jaxa.repo.nii.ac.jp:00004953,
 author = {村上, 弘志 and 北本, 俊二 and Murakami, Hiroshi and Kitamoto, Shunji},
 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 observed the first unidentified TeV gamma-ray source TeV J2032+4130 with Suzaku. With the high sensitivity for detection of diffuse X-ray emission, we found a structure in the TeV emitting region, which is coincident with a gamma-ray pulsar. By subtracting the contribution of point sources estimated by Chandra observation, we obtained X-ray spectrum of diffuse component. The spectrum can be reproduced by a power-law model with a photon index of approximately 2, and an X-ray flux of 2 x 10(exp -13) erg s(exp -1) cm(exp -2). The ratio of the gamma-ray flux to the X-ray flux is approximately 10. If the origin of TeV gamma-ray is inverse Compton scattering of microwave background by TeV electrons, which are responsible to synchrotron emission, this ratio corresponds to the magnetic field of approximately 1 micro-G., 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: AA0064574021, レポート番号: JAXA-SP-09-008E},
 pages = {54--55},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Suzaku observation of the unidentified gamma-ray source TeV J2032+4130},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}