Abstract
The similarities between blazars and radio-loud narrow-line Seyfert 1 galaxies (RLNLS1s) have received much attention. In this paper, by using the magnetized slim disk model, we calculate the jet power and disk luminosity. It is found that the jet power is only a very small fraction of the disk luminosity, <10%. This indicates that the jet orientation of RLNLS1 is close to the line-of-sight, which is similar to blazars.
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References
Abdo, A. A. et al. 2009, Astrophys. J., 707, L142.
Jiang, N. et al. 2012, Astrophys. J., 759, L31.
Komossa, S. et al. 2006, Astronomic. J., 132, 531.
Li, S., Cao, X. 2009, MNRAS, 400, 1734.
Paliya, V. S. et al. 2013, MNRAS, 428, 2450.
Yuan, W. et al. 2008, Astrophys. J., 685, 801.
Zhang, J. et al. 2013, ApJ, 774, L5.
Acknowledgements
The authors would like to thank the National Basic Research Programme (973 Programme) of China under Grant 2009CB824800, the National Natural Science Foundation of China under Grant Nos 11143003 and 11073015, and the Natural Science Foundation of Fujian Province of China (No. 2011J01023).
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Ma, R., Ping, C. Are Radio-Loud Narrow-Line Seyfert 1 Galaxies Blazar-like?. J Astrophys Astron 35, 391–392 (2014). https://doi.org/10.1007/s12036-014-9238-4
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DOI: https://doi.org/10.1007/s12036-014-9238-4