radio pulsar

The Pulsar Observation and Research with 50m Radio Telescope

用50m射电望远镜作脉冲星观测与研究

Apriori we do not know the exact distance, spin frequency, and orbital parameters of the radio pulsar that might be hidden in a data set.

因为我们不知道可能隐藏在数据集中的脉冲星的确切距离、自旋频率和轨道参数。

The cooperation program between China, Australia and Great Britain, Pulsar timing observation at 18 cm using 25 m radio telescopy of Urumqi, is introduced for its significance, reconstruction of the receiver and its sensitivity.

对正在执行的由中、澳、英合作的利用乌鲁木齐25m射电望远镜在18cm波段上进行脉冲星脉冲到达时间的观测研究项目，就其课题意义、接收系统的技术改造和观测灵敏度等进行了介绍。

Theories of Magnetosphere and Radiation Mechanism of Radio Pulsar

射电脉冲星的磁层与辐射机制理论

Last year, astronomers at the National Radio Astronomy Observatory in Charlottesville, Virginia, discovered the first pulsar orbited by two other shrunken stars, called white dwarfs.

去年在弗吉尼亚州夏洛茨维尔，国家射电天文台（National Radio Astronomy Observatory）的天文学家发现了一颗脉冲星，绕着它运动的另外两颗缩小的恒星被称为白矮星，而这一现象是前所未见的。

The 50m radio telescope of the National Astronomical Observatories will work for pulsar observations.

国家天文台正在研制的50m射电望远镜将投入脉冲星观测与研究，推动我国的脉冲星工作。