The Spectral Energy Distributions of Narrow-Line Seyfert 1 Galaxies(Session 7 : NLS1, a Mile Stone)

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概要

• 論文の詳細を見る

• Narrow-line Seyfert 1 galaxies are identified by their uniform optical spectral properties. Studies of samples of NLSls reveal, however, a range of X-ray spectral and variability behavior, and UV spectral behavior. We describe the range of behavior observed, illustrating with a comparison of the XMM-Newton and HST data from the NLS1s 1H 0707-495 and Ton S180, and discuss how the spectral energy distribution may causally link the UV and X-ray properties.

• 一般社団法人日本物理学会の論文
• 2004-11-15

著者

• LEIGHLY Karen

  Department of Physics and Astronomy, The University of Oklahoma

• Leighly Karen

  Department Of Physics And Astronomy The University Of Oklahoma

関連論文

• Discovery of Short-Timescale Variability of Seyfert 2 Galaxy NGC 6300 with XMM-Newton(Poster)
• The Spectral Energy Distributions of Narrow-Line Seyfert 1 Galaxies(Session 7 : NLS1, a Mile Stone)
• Discovery of Short-Timescale Variability of Seyfert 2 Galaxy NGC 6300 with XMM-Newton(Poster)
• XMM-Newton Observations of Luminous Narrow-Line Seyfert 1 Galaxies(Poster)
• The Spectral Energy Distributions of Narrow-Line Seyfert 1 Galaxies(Session 7 : NLS1, a Mile Stone)

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