Abstract
We have studied the correlations between luminosities (L R, L IR, L γ) in the radio, near-infrared and γ-ray wave bands for HSP TeV BL Lacs. The results show that there are significant intrinsic correlations between L R and L γ and between L IR and L γ in all states (high/average/low), and suggest that for HSP TeV BL Lacs, the Synchrotron Self-Compton radiation (SSC) is the main mechanism of high energy γ-ray emission, and the inverse Compton scattering of circum-nuclear dust is likely to be an important complementary mechanism.
Similar content being viewed by others
References
Abdo, A. A. et al. 2010a, Astrophys. J. Suppl., 188, 405.
Abdo, A. A. et al. 2010b, Astrophys. J., 716, 30.
Abdo, A. A. et al. 2012, Astrophys. J. Suppl., 199, 31.
Ackermann, M. et al. 2011a, Astrophys. J., 743, 171.
Ackermann, M. et al. 2011b, Astrophys. J., 741, 30.
Cheng, K. S., Zhang, X., Zhang, L. 2000, Astrophys. J., 537, 80.
Fan, J. H. et al. 1998, Astron. Astrophys., 338, 27.
Ghirlanda, G. et al. 2011, Mon. Not. R. Astron. Soc., 413, 852.
Ghisellini, G., Maraschi, L. 1986, Astrophys. J., 310, 317.
Ghisellini, G., Madau, P. 1996, Mon. Not. R. Astron. Soc., 280, 67.
Leon-Tavares, J. 2012, Astrophys. J., 754, 23.
Linford, J. D. et al. 2012, Astrophys. J., 744, 177.
Machalski, J., Jamrozy, M. 2006, Astron. Astrophys., 454, 95.
Maraschi, L. et al. 1992, Astrophys. J., 397, 5.
Nieppola, E. et al. 2011, Astron. Astrophys., 397, 5.
Padovani, P. 1992, Astron. Astrophys., 256, 399.
Sikora, M., Begelman, M. C., Rees, M. J. 1994, Astrophys. J., 421, 153.
Xie, G. Z., Zhang, Y. H. 1997, Astrophys. J., 477, 114.
Xie, G. Z. et al. 1998, Astrophys. J., 508, 180.
Xiong, D. R. et al. 2012, Astrophys. Space Sci., 343, 345.
Zhang, L., Cheng, K. S. 1997, Astrophys. J., 488, 9.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Xiong, D., Zhang, X. & Zheng, Y. Multi-Wave Luminosity of High-Synchrotron-Peaked TeV BL Lacs Detected by Fermi LAT. J Astrophys Astron 35, 237–240 (2014). https://doi.org/10.1007/s12036-014-9202-3
Published:
Issue Date:
DOI: https://doi.org/10.1007/s12036-014-9202-3