Similarity of Jet Radiation between Flat Spectrum Radio Quasars and GeV Narrow-Line Seyfert 1 Galaxies: A Universal $\delta$-$L_{\rm c}$ Correlation
Yong-Kai Zhu, Jin Zhang, Hai-Ming Zhang, En-Wei Liang, Da-Hai Yan, Wei, Cui, Shuang-Nan Zhang

TL;DR
This study reveals a universal correlation between Doppler factors and peak luminosities in FSRQs and GeV NLS1s, suggesting similar particle acceleration mechanisms and providing an empirical way to estimate jet Doppler boosting.
Contribution
It demonstrates a universal $oldsymbol{ ext{delta}}$-$oldsymbol{L_{ m c}}$ correlation across different blazar types and flux stages, linking observed luminosity variations to Doppler boosting effects.
Findings
FSRQ and NLS1s follow the same $oldsymbol{ ext{delta}}$-$L_{ m c}$ correlation.
The correlation holds when replacing $L_{ m c}$ with $L_{ m LAT}$.
Estimated Doppler factors for 484 FSRQs range from 3 to 41, median 16.
Abstract
By modeling the broadband spectral energy distributions (SEDs) of a typical flat spectrum radio quasar (FSRQ, 3C 279) and two GeV narrow-line Seyfert 1 galaxies (NLS1s, PMN J0948+0022 and 1H 0323+342) in different flux stages with the one-zone leptonic models, we find a universal correlation between their Doppler factors () and peak luminosities () of external Compton scattering bumps. Compiling a combined sample of FSRQs and GeV NLS1s, it is found that both FSRQs and GeV NLS1s in different stages and in different sources well follow the same - correlation. This indicates that the variations of observed luminosities may be essentially due to the Doppler boosting effect. And the universal - relation between FSRQs and GeV NLS1s in different stages may be further evidence that the particle acceleration and radiation mechanisms for…
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