Science. 1980 May 2;208(4443):495-7. doi: 10.1126/science.208.4443.495.
A full 12-hour synthesis at 6-centimeter wavelength with the Very Large Array confirms the major features previously reported for the double quasar 0957+561. In addition, the existence of radio jets apparently associated with both quasars is demonstrated. Gravitational lens models are now favored on the basis of recent optical observations, and the radio jets place severe constraints on such models. Further radio observations of the double quasar are needed to establish the expected relative time delay in variations between the images.
利用甚大阵进行了长达 12 小时的 6 厘米波段观测,结果证实了双类星体 0957+561 的先前已报告的主要特征。此外,还证明了与两个类星体都有明显联系的射电喷流的存在。根据最近的光学观测结果,现在更倾向于采用引力透镜模型,而射电喷流则对这些模型施加了严格的限制。需要对双类星体进行进一步的射电观测,以确定预期的在两个像之间变化的相对时间延迟。