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Date and Time of the Query: 2019-06-15 T14:42:47 PDT
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For refcode 2004ApJ...607..794K:
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2004ApJ...607..794K On the Relationship between the Optical Emission-Line and X-Ray Luminosities in Seyfert 1 Galaxies S. B. Kraemer, I. M. George, D. M. Crenshaw, and J. R. Gabel Abstract. We have explored the relationship between the [O III] {lambda}5007 and the 2 - 10 keV luminosities for a sample of broad- and narrow-line Seyfert 1 galaxies (BLSy1s and NLSy1s, respectively). We find that both types of Seyfert galaxies span the same range in luminosity and possess similar [O III]/X-ray ratios. The NLSy1s are more luminous than BLSy1s when normalized to their central black hole masses, a fact attributed to higher mass accretion rates. However, we find no evidence for elevated [O III]/X-ray ratios in NLSy1s, which would have been expected if they had excess extreme-ultraviolet (EUV) continuum emission compared to BLSy1s. Also, other studies suggest that the gas in narrow-line regions (NLRs) of NLSy1s and BLSy1s spans a similar range in ionization, contrary to what is expected if those of the former are exposed to a stronger flux of EUV radiation. The simplest interpretation is that, like BLSy1s, a large EUV bump is not present in NLSy1s. However, we show that the [O III]/X-ray ratio can be lowered as a result of absorption of the ionizing continuum by gas close to the central source, although there is no evidence that intrinsic line-of-sight absorption is more common among NLSy1s, as would be expected if there were a larger amount of circumnuclear gas. Other possible explanations include (1) anisotropic emission of the ionizing radiation; (2) higher gas densities in the NLRs of NLSy1s, resulting in lower average ionization; or (3) the presence of strong winds in the nuclei of NLSy1s that may drive off much of the gas in the NLR, resulting in lower cover fraction and weaker [O III] emission. Keywords: Galaxies: Seyfert, X-Rays: Galaxies
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