Statistical Properties of Narrow-Line Seyfert 1 galaxies

Details Statistical Properties of Narrow-Line Seyfert 1 galaxies Statistical Properties of Narrow-Line Seyfert 1 galaxies

2000-05-08

arxiv.org/abs/astro-ph/0005139v1

New Astron.Rev. 44 (2000) 455-460

Astronomy and Astrophysics

Astrophysics

Invited talk presented at the Joint MPE,AIP,ESO workshop on NLS1s, Bad Honnef, Dec. 1999, to appear in New Astronomy Reviews;

Scientific paper

10.1016/S1387-6473(00)00080-4

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.

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