Radio emission of the group of stars in the Aquarius and Cetus constellations

IF 0.2 Q4 PHYSICS, MULTIDISCIPLINARY
Anton A. Lipovka , Neonila M. Lipovka
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引用次数: 0

Abstract

In the present work, the optical identification of a group of radio sources located in the Aquarius and Cetus constellations in a field with the size of 1.2 square degrees has been carried out. Ten radio sources under investigation were identified with stars and one object was identified with a diffuse image (ESO-538-10). It should be stressed that eight radio objects were found to have a non-thermal radio spectrum. This fact is likely to indicate the presence of the significant magnetic field in the atmosphere of the sources. Precise radio and optical coordinates of the identified objects were suggested. Significant radio refraction in the interstellar medium in the tested space direction was revealed.

水瓶座和鲸鱼座群星群的无线电发射
本文对位于宝瓶座和鲸座的一组射电源在1.2平方度的场域中进行了光学识别。十个正在调查的射电源被确定为恒星,一个物体被确定为漫射图像(ESO-538-10)。应该强调的是,有8个无线电物体被发现具有非热无线电频谱。这一事实很可能表明在源的大气中存在着显著的磁场。提出了确定目标的精确无线电和光学坐标。在被测空间方向的星际介质中发现了显著的射电折射。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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