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首页> 外文期刊>The Astrophysical journal >SUZAKU OBSERVATIONS OF ACTIVE GALACTIC NUCLEI DETECTED IN THE SWIFT BAT SURVEY: DISCOVERY OF A 'NEW TYPE' OF BURIED SUPERMASSIVE BLACK HOLES
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SUZAKU OBSERVATIONS OF ACTIVE GALACTIC NUCLEI DETECTED IN THE SWIFT BAT SURVEY: DISCOVERY OF A 'NEW TYPE' OF BURIED SUPERMASSIVE BLACK HOLES

机译:在SWIFT BAT调查中发现的活动银河系核素的SUZAKU观测:发现一种“新型”潜油超大量黑洞

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We present the Suzaku broadband observations of two AGNs detected by the Swift BAT hard X-ray (> 15 keV) survey that did not have previous X-ray data, SWIFT J0601.9-8636 and SWIFT J0138.6-4001. The Suzaku spectra reveal in both objects a heavily absorbed power-law component with a column density of N_H approx= 10~(23.5)-10~(24) cm~(-2) that dominates above 10 keV and an intense reflection component with a solid angle approx> 2π from a cold, optically thick medium. We find that these AGNs have an extremely small fraction of scattered light from the nucleus, approx< 0.5% with respect to the intrinsic power-law component. This indicates that they are buried in a very geometrically thick torus with a small opening angle and/or have an unusually small amount of gas responsible for scattering. In the former case, the geometry of SWIFT J0601.9 -8636 should be nearly face-on as inferred from the small absorption for the reflection component. The discovery of two such objects in this small sample implies that there must be a significant number of yet unrecognized, very Compton thick AGNs viewed at larger inclination angles in the local universe, which are difficult to detect even in the currently most sensitive optical or hard X-ray surveys.
机译:我们展示了通过Swift BAT硬X射线(> 15 keV)调查发现的两个AGN的Suzaku宽带观测结果,它们没有以前的X射线数据,SWIFT J0601.9-8636和SWIFT J0138.6-4001。 Suzaku光谱在两个物体中都显示出一个吸收很强的幂律分量,其列密度为N_H大约= 10〜(23.5)-10〜(24)cm〜(-2),在10 keV以上时占主导地位,而强反射分量为与冷的,光学上较厚的介质的立体角大约>2π。我们发现,这些AGN的原子核散射光极小,相对于本征幂律分量约小于0.5%。这表明它们被埋在几何形状非常厚的圆环中,且圆环角较小,并且/或者气体散布量非常少。在前一种情况下,SWIFT J0601.9 -8636的几何形状应几乎面朝上,这是从反射组件的小吸收量得出的。在这个小样本中发现了两个这样的物体,这意味着在本地宇宙中以较大的倾斜角度观察​​时,必须存在大量尚未发现的,非常康普顿厚的AGN,即使在目前最灵敏的光学或硬观测中也很难检测到。 X射线调查。

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