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Clues on Blazars Phenomenology from the FIRST Flat Spectrum Sample

机译:来自第一个平面谱样本的布拉齐人类现象学的线索

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We highlight some results of our work on the FIRST Flat Spec-trum Sample (FFSS) of blazars, in particular concerning the relationship be-tween their luminosity and Spectral Energy Distribution (SED), including pre-liminary results on the power of the emission of their Broad Line Region (BLR). The current analysis shows that within the FFSS, which captures at once a broad range of blazar phenomenology, the SED-power correlation which con-stituted the observational basis of the blazar sequence hypothesis seems to be present. We also find that FFSS BL Lac and FSRQ sources, despite having been been selected together, tend to stay separate with respect to several properties, such as SED type and luminosities (e.g. radio, y-ray, BLR). The BLR analysis suggests that in BL Lac objects the BLR is indeed under-luminous compared with. FSRQ. This in turn suggests that ratio between thermal and norm-thermal emission in the two classes of objects is different. Finally, we discuss sonic clues emerging from the study of the sample of blazars detected at GeV y-rays by Fermi/LAT, focusing again on the question of power of SED properties.
机译:我们强调对耀变体的第一平的规格,TRUM样品(FFSS)我们工作的一些成果,特别是有关的关系是吐温的亮度和光谱能量分布(SED),包括在发射的功率预liminary结果他们的宽线区(BLR)。目前的分析表明,该FFSS,内一次广泛耀变现象的捕获,这CON-stituted的耀变体序列假设的观测基础的SED-功率相关性似乎是本。我们还发现,FFSS BL紫胶和FSRQ源,尽管已被一起选择,倾向于保持分离相对于几个属性,诸如SED类型和光度(例如无线电,γ射线,BLR)。最优惠贷款利率的分析表明,在BL Lac天体最优惠利率的确在发光相比。 FSRQ。这又表明在两类对象的热和准则热发射之间的比率是不同的。最后,我们讨论声线索从耀变体样品的研究得出费米在GeV的γ射线检测/ LAT,对SED性质的权力问题再次聚焦。

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