The Eddington Ratio of H 2 O Maser Host AGN |
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Authors: | Q. Guo J. S. Zhang J. Wang |
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Affiliation: | 1. Hunan University of Humanities, Science and Technology, Loudi, 417000, China 2. Center for Astrophysics, Guangzhou University, Guangzhou, 510006, China
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Abstract: | The Eddington ratio λ was derived for the entire maser host AGN sample, based on the intrinsic X-ray luminosity, the X-ray bolometric correction C X and the mass of central black hole. Further the [O III] bolometric correction C [O III] was estimated for our sample. Possible relations were also investigated between the maser luminosity and the bolometric luminosity – the Eddington ratio. |
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