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Extragalactic radio sources with sharply inverted spectrum at metre wavelengths

机译:河外无线电源,在米处有明显反转的光谱   波长

摘要

We present the first results of a systematic search for the rareextragalactic radio sources showing an inverted (integrated) spectrum, withspectral index $\alpha \ge +2.0$, a previously unexplored spectral domain. Thesearch is expected to yield strong candidates for $\alpha \ge +2.5$, for whichthe standard synchrotron self-absorption (characterized by a single power-lawenergy distribution of relativistic electron population) would not be aplausible explanation, even in an ideal case of a perfectly homogeneous sourceof incoherent synchrotron radiation. Such sharply inverted spectra, if found,would require alternative explanations, e.g., free-free absorption, ornon-standard energy distribution of relativistic electrons which differs from apower-law (e.g., Maxwellian). The search was carried out by comparing two sensitive low-frequency radiosurveys made with sub-arcminute resolution, namely, the WISH survey at 352 MHzand TGSS/DR5 at 150 MHz. The overlap region between these two surveys contains7056 WISH sources classified as `single' and brighter than 100 mJy at 352 MHz.We focus here on the seven of these sources for which we find $\alpha > +2.0$.Two of these are undetected at 150 MHz and are particularly good candidates for$\alpha > +2.5$. Five of the seven sources exhibit a`Gigahertz-Peaked-Spectrum' (GPS).
机译:我们提供了系统搜索稀有外拉式无线电源的第一结果,该无线电源显示了一个倒置的(积分的)光谱,光谱索引为$ \ alpha \ ge + 2.0 $,以前是未探索的光谱域。预计该研究将产生$ \ alpha \ ge + 2.5 $的强大候选者,即使在理想的情况下,标准的同步加速器自吸收(由相对论电子种群的单一幂律能量分布表征)也不是合理的解释。非相干同步加速器辐射的完全均匀的源。如果发现了这种急剧反转的光谱,则将需要其他解释,例如,自由能吸收或相对论电子的非标准能量分布,其不同于幂律(例如麦克斯韦定律)。搜索是通过比较两个以亚弧度分辨率进行的敏感的低频无线电测量进行的,即352 MHz的WISH测量和150 MHz的TGSS / DR5。这两个调查的重叠区域包含7056个WISH信号源,在352 MHz下被分类为``单个''且比100 mJy亮。我们在此重点关注其中七个我们发现$ \ alpha> + 2.0 $的信号源,其中两个未被发现在150 MHz时,尤其适合$ \ alpha> + 2.5 $。七个来源中有五个展示了“千兆赫峰频谱”(GPS)。

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