论文标题
新脉冲星的无线电排放率在111 MHz
Peculiarities of radio emission from new pulsars at 111 MHz
论文作者
论文摘要
提出了在Pushchino射电天文台发现的三个新脉冲星的无线电发射的分析。详细的观察结果是使用大阶段阵列（LPA）以111 MHz的频率进行，总带宽为2.245 MHz，时间分辨率为2.46或5.12 ms。所有脉冲星均表现出其辐射的特征，在J0220+3622中观察到子孔漂移，在J0303+2248中显示了耀斑活性，并且在J0810+3725中检测到无效现象。
The analysis of radio emission of three new pulsars discovered at the Pushchino Radio Astronomy Observatory is presented. The detailed observations were carried out at a frequency of 111 MHz using the Large Phased Array (LPA) and the standard digital receiver with a total bandwidth is 2.245 MHz and time resolution is 2.46 or 5.12 ms. All pulsars exhibit features of their radiation, the subpulse drift is observed in J0220+3622, the flare activity is exhibited in J0303+2248 and the nulling phenomenon has been detected in J0810+3725.
