Is There a Link Between Emission-Line Widths and X-Ray Continuum Slopes in Narrow Line Seyfert 1 Galaxies?
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Abstract
We present the discovery of 18 narrow line Seyfert 1 galaxies (NLS1).The optical spect rashow the Balmer lines only slightly broader than the forbidden lines and contain strong Fe Ⅱ emission.No particularly soft X-ray spectral slopes can be seen compared to a normal Seyfert 1 galaxies sample.
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