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- W2100091390 abstract "The maximal jet power can be extracted from a standard thin accretion disk/spinning black hole is calculated as a function of dimensionless accretion rate dotm (dotm=dotM/dotMEdd). Comparing with the jet power derived from the extended radio luminosity, we find that the accretion disks in most BL Lac objects should not be standard accretion disks. It is found that a pure ADAF is too faint to produce the optical ionizing luminosity of BL Lac objects derived from their narrow-line luminosity. We propose that an ADAF is present in the inner region of the disk and it transits to a standard thin disk outside the radius Rtr in most BL Lac objects, i.e., ADAF+SD (standard disk) scenario. This scenario can explain both the jet power and optical ionizing continuum emission of these BL Lac objects. The inferred Rtr ∼ 40-150 GMbh/c2, if the disks are accreting at the rate dotm=0.01." @default.
- W2100091390 created "2016-06-24" @default.
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- W2100091390 date "2004-01-01" @default.
- W2100091390 modified "2023-09-26" @default.
- W2100091390 title "Disk-Jet Connection in BL Lac Objects with Different Accretion Modes" @default.
- W2100091390 doi "https://doi.org/10.1143/ptps.155.319" @default.
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