Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..245..243f&link_type=abstract
Formation and Evolution of Galaxy Bulges, Proceedings of the International Astronomical Union, IAU Symposium, Volume 245, p. 243
Astronomy and Astrophysics
Astronomy
1
Scientific paper
In this paper, we used the method to determine the central black mass (M), and the boosting factor (δ), the propagation angle (Φ), and the distance along the axis to the site of the γ-ray production (d) as well for 32 γ-ray loud blazars with available variability timescales. If we take the intrinsic γ-ray luminosity to be λ times the Eddington luminosity, i.e. Lγin=λ{LEdd}, then we have following results: the masses of the black hole are in the range of (0.9 ~ 101)×107M&sun;(λ = 1.0) or (1.30 ~ 153)×107M&sun;(λ=0.1).
Fan Junhui H.
Gao Yanfang
Hua Tong Xu
Huang Yong-Yi
Liu Ya-Ying
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