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Bolometric Luminosity Correction of H2O Maser AGNs

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Abstract

For the H2O maser host AGN sample, we derived their bolometric luminosity corrections, based on their X-ray data and [O III] emission line luminosities. Our results for maser AGNs is comparable to that of non-maser AGNs.

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Acknowledgements

This work is supported by the National Natural Science Foundation of China (NSFC 11178009), Hunan Provincial Natural Science Foundation of China (10JJ3020), and the research fund of Hunan University of Arts and Science (JJZD 201101).

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Authors and Affiliations

  1. Hunan University of Humanities, Science and Technology, Loudi, 417000, China

    Q. Guo

  2. Center for Astrophysics, Guangzhou University, Guangzhou, 510006, China

    Q. Guo, J. S. Zhang & J. Wang

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  1. Q. Guo
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  2. J. S. Zhang
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  3. J. Wang
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Correspondence to J. S. Zhang.

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Guo, Q., Zhang, J.S. & Wang, J. Bolometric Luminosity Correction of H2O Maser AGNs. J Astrophys Astron 35, 223–225 (2014). https://doi.org/10.1007/s12036-014-9199-7

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  • DOI: https://doi.org/10.1007/s12036-014-9199-7

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