The Eddington Ratio of H 2 O Maser Host AGN

Details The Eddington Ratio of H 2 O Maser Host AGN The Eddington Ratio of H 2 O Maser Host AGN

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011japa...32...49g&link_type=abstract

Journal of Astrophysics and Astronomy, Volume 32, Issue 1-2, pp. 49-51

Astronomy and Astrophysics

Astrophysics

Eddington Ratio, Bolometric Correction, Maser, Eddington Ratio—Bolometric Correction—Maser

Scientific paper

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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