Department of High Energy Astrophysics, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA)
Department of High Energy Astrophysics, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA)
Department of High Energy Astrophysics, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA)
Department of Applied Physics, University of Miyazaki
Department of Physical Science, Hiroshima University
出版者
宇宙航空研究開発機構
出版者（英）
Japan Aerospace Exploration Agency (JAXA)
雑誌名
宇宙航空研究開発機構特別資料:
雑誌名(英)
JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H
巻
JAXA-SP-09-008E
ページ
46 - 47
発行年
2010-02-26
会議概要（会議名, 開催地, 会期, 主催者等）（英）
The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan
抄録（英）
We studied nature of the pulsar wind nebulae (PWNe) whose association to the TeV gamma-ray sources is suspected. A total of 16 PWNe was selected and their X-ray data were analyzed. We found that the parameters of the TeV associated PWNe are basically same as those not detected in the TeV band. Although the energy loss time scale of the X-ray emitting, high-energy electrons in the PWNe is only approximately 2 kyr, we found that the size of the X-ray emission region of the TeV PWNe keeps increasing up to approximately 100 kyr. Two possibilities are discussed for this continued increase of the X-ray sizes.
内容記述（英）
Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science
An X-ray Study of the Pulsar Wind Nebulae Discovered in the Very High Energy Gamma-ray Band
64574017.pdf
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