Statistical Properties of Narrow-Line Seyfert 1 galaxies
arXiv:astro-ph/0005139 · doi:10.1016/S1387-6473(00)00080-4
Abstract
The number of publications considering Narrow-Line Seyfert 1 galaxies has increased dramatically in recent years. Especially after the launch of the X-ray missions ROSAT and ASCA, Narrow-Line Seyfert 1s have become very popular. In these proceedings I will give an overview of how they are distributed over the electromagnetic spectrum. I will describe what we know about them at radio, infrared, optical, and X-ray bands, and how they differ and how they are similar to Broad-Line Seyfert 1s. Finally I will introduce a method to find them with high probability.
Invited talk presented at the Joint MPE,AIP,ESO workshop on NLS1s, Bad Honnef, Dec. 1999, to appear in New Astronomy Reviews; also available at http://wave.xray.mpe.mpg.de/conferences/nls1-workshop
References in corpus (4)
- A Comprehensive Spectral and Variability Study of Narrow-Line Seyfert 1 Galaxies Observed by ASCA: II. Spectral Analysis and Correlations
- A Comprehensive Spectral and Variability Study of Narrow-Line Seyfert 1 Galaxies Observed by ASCA: I. Observations and Time Series Analysis
- X-ray Spectra of the RIXOS source sample
- New Mid-Infrared Diagnostic of the Dusty Torus Model for Seyfert Nuclei
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- Statistical properties of local active galactic nuclei inferred from the RXTE 3-20 keV all-sky survey
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- First XMM-Newton study of two Narrow-Line Seyfert 1 galaxies discovered in the Sloan Digital Sky Survey
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- Hunting for the nature of the enigmatic narrow-line Seyfert 1 galaxy PKS 2004-447
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