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首页> 外文期刊>The astronomical journal >The Interacting Late-type Host Galaxy of the Radio-loud Narrow-line Seyfert 1 IRAS 20181-2244
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The Interacting Late-type Host Galaxy of the Radio-loud Narrow-line Seyfert 1 IRAS 20181-2244

机译:无线电响的窄线赛弗1 IRAS的交互晚期型宿主银河20181-2244

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Narrow-line Seyfert 1 galaxies (NLS1s) are a class of active galactic nuclei that are known to be one of the few sources of γ-rays, which originate in a relativistic beamed jet. Because of their relatively large distance, a poorly investigated aspect of these jetted NLS1s is their environment, and in particular, their host galaxy. In this work, we present the results of a morphological analysis of the host galaxy of the jetted NLS1 IRAS 20181-2244 observed with the 6.5 m Baade Telescope of the Las Campanas Observatory. The GALFIT analysis run on the Ks image, along with additional spectroscopic observations performed with the Nordic Optical Telescope, clearly revealed the presence of an interacting system of two galaxies. The data suggest that this NLS1 is hosted by a late-type galaxy, although the result is not conclusive. This analysis, along with other results in the literature, might suggest that two populations of jetted NLS1 exist. Further morphological studies are needed to confirm or disprove this hypothesis.
机译:窄线塞弗1星系(NLS1s)是一类活跃的银河核,已知是为相对论性射流产生的少数γ射线源之一。由于距离相对较大,这些喷出的NLS1的研究不足,是它们的环境,尤其是它们的宿主星系。在这项工作中,我们提供了用拉斯坎帕纳斯天文台6.5 m巴德望远镜观测到的喷射NLS1 IRAS 20181-2244宿主星系的形态分析结果。在Ks图像上运行的GALFIT分析以及使用北欧光学望远镜进行的其他分光镜观察清楚地揭示了两个星系相互作用系统的存在。数据表明,该NLS1由晚期型星系托管,尽管结果尚不确定。该分析以及文献中的其他结果可能表明存在两个喷射的NLS1种群。需要进一步的形态学研究来证实或证明这一假设。

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