Discovery of Short-Timescale Variability of Seyfert 2 Galaxy NGC 6300 with XMM-Newton(Poster)
スポンサーリンク
概要
- 論文の詳細を見る
We found short time variability (Δt 〜 1 ks) of NGC 6300 in the 2-10 keV band with XMM-Newton. Its normalized power spectral density can be expressed by a power-law function of frequency with a slope of 〜-1.7. These results are similar to those of Seyfert 1 galaxies. Using the relation between time variability and central black hole mass, we estimate the black hole mass of about 3×10^5 M_<⊙>. The time variability analysis suggests that NGC 6300 actually has a Seyfert 1 nucleus obscured by a thick matter.
- 理論物理学刊行会の論文
- 2004-11-15
著者
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Matsumoto Chiho
Department of Biotechnology and Life Science, Tokyo University of Agriculture and Technology
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HAYASHIDA Kiyoshi
Department of Earth and Space Science, Graduate School of Science, Osaka University
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AWAKI Hisamitsu
Department of Physics, Ehime University
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Murakami Hiroyuki
Japan Aerospace Exploration Agency Institute Of Space And Astronautical Science
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HIYOSHI Kenji
Meisei Electric Company
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Murakami H
Japan Aerospace Exploration Agency Kanagawa
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Hayashida Kiyoshi
Department Of Earth And Space Science Osaka University
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Hayashida K
Department Of Earth And Space Science Osaka University
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Hashimotodani K
Department Of Earth And Space Science Graduate School Of Science Osaka University
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Hayashida Kiyoshi
Department Of Astrophysics Osaka University
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MURAKAMI Hirokatsu
Department of Physics, Ehime University
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LEIGHLY Karen
Department of Physics and Astronomy, The University of Oklahoma
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GRUPE Dirk
Astronomy Department, The Ohio State University
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Hayashida Kiyoshi
Department Of Earth And Space Science Faculty Of Science Osaka University
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Awaki H
Department Of Physics Ehime University
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Awaki Hisamitsu
Department Of Physics Ehime University
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Grupe Dirk
Astronomy Department The Ohio State University
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Leighly Karen
Department Of Physics And Astronomy The University Of Oklahoma
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Hamaguchi Kenji
Department Of Physics Faculty Of Science Kyoto University
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Matsumoto C
Division Of Energy Science Ecotopia Science Institute Nagoya University
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Matsumoto Chiho
Department Of Biotechnology And Life Science Tokyo University Of Agriculture And Technology
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Matsumoto Chiho
Division Of Energy Science Ecotopia Science Institute Nagoya University
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Murakami Hirokatsu
Department Of Physics Graduate School Of Science Kyoto University
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