We collect 16 gamma-ray-loud blazars (seven BL Lac objects and nine flat-spectrum radio quasars) with both observed near-infrared and gamma-ray flux densities and find that the near-IR luminosity correlates better with gamma-ray luminosity than with X-ray. Possible constraints on the gamma-ray emission mechanism are discussed. We suggest that the gamma-ray radiation is probably created by inverse Compton scattering of the radiation from hot circumnuclear dust by beamed, ultrarelativistic electrons.
Xie GZ,Zhang YH,Fan, JH,et al. The relation between gamma-ray and near-infrared radiation in gamma-ray-loud blazars[J]. ASTROPHYSICAL JOURNAL,1997,477(1):114-117.
APA
谢光中,张有宏,Fan, JH,&Xie, GZ.(1997).The relation between gamma-ray and near-infrared radiation in gamma-ray-loud blazars.ASTROPHYSICAL JOURNAL,477(1),114-117.
MLA
谢光中,et al."The relation between gamma-ray and near-infrared radiation in gamma-ray-loud blazars".ASTROPHYSICAL JOURNAL 477.1(1997):114-117.
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