Multiwavelength Doppler factors for Fermi-detected gamma-ray loud blazars

被引:2
|
作者
Zeng, Hou-Dun [1 ]
Zhang, Li [1 ]
机构
[1] Yunnan Univ, Dept Phys, Kunming 650091, Peoples R China
关键词
galaxies: active; galaxies: nuclei; galaxies: jets; radiation mechanisms: non-thermal; BL-LACERTAE OBJECTS; ACTIVE GALACTIC NUCLEI; RELATIVISTIC JETS; COMPTON; EMISSION; QUASARS; SPECTRA; MODEL;
D O I
10.1088/1674-4527/11/4/002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We collect a sample of 51 Fermi-detected gamma-ray loud blazars with known radio Doppler factors and study properties of the Doppler factors of blazars at optical, X-ray and gamma-ray bands. A basic assumption is that the emission from the radio to gamma-ray bands of the blazars are produced by the nonthermal radiation of accelerated particles in a jet. Our results show that (1) the Doppler factors of blazars are a function of frequency, with the Doppler factor decreasing with frequency from the radio to X-ray regions, and then increasing from the X-ray to gamma-ray regions which are similar to results given by Zhang et al., and (2) there are marginal correlations between the Doppler factors at radio and X-ray bands and the synchrotron peak frequency, and a strong correlation between the Doppler factor in the gamma-ray band and the synchrotron peak frequency, but no correlation in the optical band.
引用
收藏
页码:391 / 400
页数:10
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