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THE BEAMING PATTERN OF DOPPLER-BOOSTED THERMAL ANNIHILATION RADIATION: APPLICATION TO MEV BLAZARS

机译:多普勒增强的热AN灭辐射的辐射图案:在梅夫布拉泽斯上的应用

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The beaming pattern of thermal annihilation radiation is broader than the beaming pattern produced by isotropic nonthermal electrons and positrons in the jets of radio-emitting active galactic nuclei that Compton scatter photons from an external isotropic radiation field. Thus, blueshifted thermal annihilation radiation can provide the dominant contribution to the high-energy radiation spectrum at observing angles θ approx > 1/Γ, where Γ is the bulk Lorentz factor of the outflowing plasma. This effect may account for the spectral features of MeV blazars discovered with the Compton Telescope on the Compton Gamma Ray Observatory. Coordinated gamma-ray observations of annihilation line radiation to infer Doppler factors and VLBI radio observations to measure transverse angular speeds of outflowing plasma blobs can be used to determine the Hubble constant.
机译:热an灭辐射的光束方向图比康普顿从外部各向同性辐射场散射光子的放射活性银河核射流中的各向同性非热电子和正电子产生的光束方向图更宽。因此,蓝移的热radiation灭辐射可以在观察角θ大约> 1 /Γ的情况下对高能辐射谱起主要作用,其中Γ是流出等离子体的整体洛伦兹因子。这种影响可能解释了在康普顿伽玛射线天文台上用康普顿望远镜发现的MeV blazar的光谱特征。 an灭线辐射的协调伽马射线观测可以推断多普勒因子,而VLBI射电观测可以测量流出的等离子体斑点的横向角速度,可以用来确定哈勃常数。

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