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Abstract

We collect 214 Seyfert 1 galaxies(147 narrow line Seyfert 1 and 67 broad line Seyfert 1) and research black hole mass bulge velocity dispersion Eddington radio luminosity at 5100 Å and redshift. Our conclusions are follows: (1) when computing black hole mass, we should consider the effect of radiation pressure, especially for the narrow line Seyfert 1 galaxies; (2) when the effect of radiation pressure is considered, narrow line Seyfert 1 galaxies meet MBH-σ relation of normal galaxies and are in su-Eddington accretion; (3) in a large samples, the evolution of Seyfert 1 galaxies is from narrow line Seyfert 1 galaxies to broad line Seyfert 1 galaxies, which is consistent with other results obtained in different ways.

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1.
Funds:Project supported by the National Natural Science Foundation of China (Grant No. 11163007), the Gravitational Theory Innovation Team of Yunnan Provincial of China and High Energy Astrophysics of University Innovation Team of Yunnan Provincial of China.

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Vol. 61, Issue 22 - 2012-11-20

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