Investigation of the Millisecond Pulsar Origins by their Spin Periods at the Wavebands of Radio, X-Ray, and gamma-Ray
Investigation of the Millisecond Pulsar Origins by their Spin Periods at the Wavebands of Radio, X-Ray, and gamma-Ray
复制标题
通过射电、X 射线和 γ 射线波段的自旋周期研究毫秒脉冲星的起源
DOI：
10.1088/1538-3873/aaecc7
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发表时间：
2019
影响因子：
3.5
通讯作者：
Wang Shuang-Qiang
中科院分区：
文献类型：
--
作者：
Wang De-Hua;Zhang Cheng-Min;Wang Shuang-Qiang
为了跟踪银河场中由吸积和自转驱动的毫秒脉冲星(MSPS)的形成和演化过程，我们研究了自旋周期(P)和自旋下降功率(P)。
To track the formation and evolution links of the millisecond pulsars (MSPs) powered by accretion and rotation in the Galactic field, we investigate the spin period (P) and spin-down power (