来自NVSS和FIRST的可变射电源光学特性

H. Abrahamyan, A. Mickaelian, G. Paronyan, G. Mikayelyan
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引用次数: 0

摘要

我们已经进行了许多研究来揭示活动星系的无线电特性,即AGN和星暴。一项主要工作涉及到NVSS和FIRST无线电目录的相互关系和可变射电源的揭示。最有可能的是,它们中的大多数都是银河系外的;AGN和星暴。我们对其中的6301个天体进行了光谱分类,发现了许多塞弗特、liner和星暴。我们还研究了VCV-13 AGN、马卡里安星系和Blazars的射电特性。我们研究的目的之一是建立在射电中探测到的正常星系和射电活跃星系之间的射电/光通量比极限。这些研究的最终目标是将射电研究结果和活动星系的射电特性与伽玛射线、x射线、紫外线、光学、红外和亚毫米/毫米相结合,对这些天体有一个整体的多波长认识。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Optical properties of variable radio sources from NVSS and FIRST
We have carried out a number of studies to reveal radio properties of active galaxies, namely AGN and Starbursts. A major work was related to the cross-correlation of NVSS and FIRST radio catalogues and revelation of variable radio sources. Most probably, most of them are extragalactic ones; AGN and Starbursts. We have carried out spectroscopic classification of 6301 of these objects and revealed many Seyferts, LINERs and Starbursts. We have also studied radio properties of VCV-13 AGN, Markarian galaxies and Blazars. One of the aims of our studies is to establish the radio/opt flux ratio limit between normal galaxies detected in radio and radio loud active galaxies. The ultimate goal of these studies is to combine results obtained from radio studies and derived radio properties of active galaxies with gammaray, X-ray, UV, optical, IR and submm/mm to have the overall multiwavelength understanding on these objects.
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