射电星系NGC326的多频率研究
天体物理学
2007-05-23 v1
摘要
我们报告了基于VLA在1.4、1.6、4.8、8.5和14.9 GHz观测的反称称射电星系NGC326的初步结果。这些数据允许我们详细探讨该特殊对象的形态、光谱和极化特性在不同空间分辨率水平上的性质。
引用
@article{arxiv.astro-ph/0012127,
title = {A multi-frequency study of the radio galaxy NGC326},
author = {M. Murgia and P. Parma and R. Fanti and H. R. de Ruiter and R. D. Ekers and E. B. Fomalont},
journal= {arXiv preprint arXiv:astro-ph/0012127},
year = {2007}
}
备注
4 pages, 3 figures, uses newpasp.sty (included). To appear in R.A. Laing and K.M. Blundell (Eds.) 'Particles and Fields in Radio Galaxies' Oxford, UK, 2000, to be published by the Astronomical Society of the Pacific (ASP)