The Spectral Energy Distributions of Narrow-line Seyfert 1 Galaxies

Details The Spectral Energy Distributions of Narrow-line Seyfert 1 Galaxies The Spectral Energy Distributions of Narrow-line Seyfert 1 Galaxies

2004-02-27

arxiv.org/abs/astro-ph/0402676v1

Prog.Theor.Phys.Suppl.155:223-230,2004

Astronomy and Astrophysics

Astrophysics

8 pages, 6 figures, 1 color figure, invited contribution for the conference "Stellar-mass, Intermediate-mass, and Supermassive

Scientific paper

10.1143/PTPS.155.223

Narrow-line Seyfert 1 galaxies are identified by their uniform optical spectral properties. Studies of samples of NLS1s 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 1H0707-495 and TonS180, and discuss how the spectral energy distribution may causally link the UV and X-ray properties.

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