A method for estimating the mass of the central bodies in active galaxy nuclei and quasars

Details A method for estimating the mass of the central bodies in active galaxy nuclei and quasars A method for estimating the mass of the central bodies in active galaxy nuclei and quasars

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pazh....8..535z&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, Sept. 1982, p. 535-537) Soviet Astronomy Letters (ISSN 0360-0327), vol. 8, Sept.-Oct

Astronomy and Astrophysics

Astronomy

Active Galactic Nuclei, Active Galaxies, Galactic Structure, Gamma Ray Astronomy, Mass Distribution, Quasars, Seyfert Galaxies, Black Holes (Astronomy), Galactic Radiation, Pair Production, Photon Density, Radio Galaxies

Scientific paper

From the lack of absorption of 1-10 MeV gamma rays in the nuclei of the radio galaxy Cen A and the Seyfert galaxy NGC 4151 and in the quasar 3C 273, lower limits are set on the mass of the central structures in these objects. Actual values for the mass should become feasible to estimate when observations of active galaxy nuclei are obtained at photon energies of at least 10 MeV.

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