Jet power extracted from ADAFs and the application to Fermi BL Lacertae objects
Chen Yongyun, Gu Qiusheng, Fan Junhui, Yu Xiaoling, Ding Nan, Guo, Xiaotong, Xiong Dingrong

TL;DR
This study models jet power in Fermi BL Lac objects using ADAF-based theories, finding that most jet powers can be explained by hybrid models, and reveals correlations between jet power, accretion rates, and emission processes.
Contribution
It applies ADAF-based jet models to Fermi BL Lacs, providing new insights into jet formation mechanisms and emission processes in these objects.
Findings
Most jet powers of IBL and HBL are explained by the hybrid ADAF model.
A higher accretion rate is observed in LBL compared to IBL and HBL.
Inverse Compton luminosity correlates with synchrotron luminosity, supporting SSC dominance.
Abstract
We calculate the jet power of the Blandford-Znajek (BZ) model and the hybrid model based on the self-similar solution of advection-dominated accretion flows (ADAFs). We study the formation mechanism of the jets of BL Lacs with known redshifts detected by the Fermi satellite after 10 yr of data (4FGL-DR2). The kinetic power of the jets of Fermi BL Lacs is estimated through radio luminosity. The main results are as follows. (1) We find that the jet kinetic power of about 72\% intermediate peak frequency BL Lacs (IBL) and 94\% high-frequency peak BL Lacs (HBL) can be explained by the hybrid jet model based on ADAFs surrounding Kerr black holes. However, the jet kinetic power of about 74\% LBL cannot be explained by the BZ jet model or the hybrid model. (2) The LBL has a higher accretion rate than IBL and HBL. About 14\% IBL and 62\% HBL have pure optically thin ADAFs. However, 7\% LBL may…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Astrophysical Phenomena and Observations · Magnetic confinement fusion research
