Abstract： We discuss jet production from an advection dominated accretion flow (ADAF) around a rotating black hole (BH) in an electromagnetic regime. An analytical expression for the jet power is derived by using an equivalent circuit in the BH magnetosphere. It turns out that a large fraction of jet powers is contributed from the inner region of the ADAF, and the jet power depends sensitively on the degree to which the flow is advection-dominated. In addition, we use our model to fit the strong jet powers of several BL Lac objects, which cannot be explained by virtue of the BZ process.
(Galactic nuclei (including black holes), circumnuclear matter, and bulges)
引用本文:
GONG Xiao-Long;WANG Ding-Xiong. An Electromagnetic Model for Jet Power from an Advection Dominated Accretion Flow around a Rotating Black Hole[J]. 中国物理快报, 2005, 22(5): 1293-1295.
GONG Xiao-Long, WANG Ding-Xiong. An Electromagnetic Model for Jet Power from an Advection Dominated Accretion Flow around a Rotating Black Hole. Chin. Phys. Lett., 2005, 22(5): 1293-1295.
2005, Vol. 22 
