Time Dependence of the Radio Emission from Cta 21 and Cta 102.

机译：Cta 21和Cta 102的无线电发射的时间依赖性。

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Sholomitskii has reported variations with a period of about 100 days and amplitude of = 23% in the 32.5 cm radio intensity of CTA 102. We have examined the Caltech observations of this source at 31.3 cm, which cover the period from its discovery in 1959 through 1961. A firm upper limit of = 10% can be set on variations with 100 day period. (Author)

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Maltby, P.; Moffet, A. T.;
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年度 1965
页码 1-10
总页数 10
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Extraterrestrial radio waves; Variable stars; Radio astronomy; Astrophysics; Brightness; Tables(Data); Measurement; Periodic variations; Cta 102;

机译：地外无线电波;变星;射电天文学;天体物理学;亮度;表（数据）;测量;周期变化; Cta 102;

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机译：射电与射电Galaxy 3C 120和Blazar CTA 102中的γ射线之间的连接
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7. The Connection between the Radio Jet and the γ-ray Emission in the Radio Galaxy 3C 120 and the Blazar CTA 102 [O] . Casadio Carolina, Gómez José, Jorstad Svetlana, 2016

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Time Dependence of the Radio Emission from Cta 21 and Cta 102.

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