IFCA (CSIC-UC)
NASA/GSFC, Code 661
Department of Physics & AstronomyUniversity of Leicester
Astrophysics Group, School of Physical & Geographical Sciences, Keele University
INAF - Osservatorio Astronomico di Brera
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
338 - 339
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）
Here we report on a Suzaku observation of the nearby BLRG 3C 111, a bright FR II with a single sided jet exhibiting superluminal motion. Preliminary results indicate that the 0.5 - 200 keV spectrum is dominated by a disklike component, with a power law with photon index approximately 1.6 cutting off around 100 keV, and a reflection R approximately 0.04. The Suzaku data do not indicate the presence of a hard X-ray component associated with the jet emission, that should become dominant at GeV energies (i.e. in the range covered by FERMI ).
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
The Suzaku view of the BLRG 3C 111
64574132.pdf
(317.4KB)
