Department of Earth and Space Science, Graduate School of Science, Osaka University
Department of Earth and Space Science, Graduate School of Science, Osaka University
Code 662, NASA Goddard Space Flight Center
Department of Earth and Space Science, Graduate School of Science, Osaka University
Department of Earth and Space Science, Graduate School of Science, Osaka University
Department of Earth and Space Science, Graduate School of Science, Osaka 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
38 - 39
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 performed a comprehensive study of the Cygnus Loop, which is one of the largest (R approximately 80 min) and the brightest supernova remnants (SNRs) in the X-ray sky. In spite that it is a middle-aged SNR (approximately 10,000 yr), there is a substantial amount of fresh metal ejected from the progenitor. We have been observing this SNR since 2002 with Suzaku and XMM-Newton observatories, and now we have 41 pointing observation data sets in total. Here we report the results of our observations.
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
Suzaku and XMM-Newton Observations of the Cygnus Loop
64574013.pdf
(326.87KB)
