PULSARS相关论文
Supernova remnants are supposed to be the most possible sources of cosmic rays.However,alternative sources of cosmic ray......
Large-scale electron-positron plasmas (EPPs) are common in the early universe and in pulsar magnetospheres and have been......
The orthogonal polarization modes (OPM) have been reported observationally and widely accepted by pulsar researchers. Ho......
We investigate the birthrate problem for low-mass X-ray binaries(LMXBs) and millisecond radio pulsars(MRPs) in this pape......
PSR B2111+46 is studied and analyzed by the method of Gaussian fit separation of the average profile (GFSAP). It has bee......
脉冲星 nulling 是为很多个时期的脉搏排放的突然的停止的现象。nulling 部分经常被用来描绘现象。我们建议一个新方法分析脉冲星 ......
Effects of dynamo magnetic fields on observational properties of accreting millisecond X-ray pulsars
In this paper,we have investigated accreting millisecond X-ray pulsars,which are rapidly rotating neutron stars in low-m......
A comparison between repeating bursts of FRB 121102 and giant pulses from Crab pulsar and its applic
There are some similarities between bursts of repeating fast radio bursts(FRBs)and giant pulses(GPs)of pulsars.To explor......
The pulse profiles of the Crab pulsar (as well as some other pulsars) vary with time.They can lead to a major source of ......
We report pulsar timing observations carried out in L-band with NTSC's 40-meter Haoping Radio Telescope(HRT),which was c......
In this paper,the propagation of x-ray bursts in the magnetoplasma of pulsar magnetosphere is discussed.The electromagne......
为探究吕家坨井田地质构造格局,根据钻孔勘探资料,采用分形理论和趋势面分析方法,研究了井田7......
PSR B2111+46 is studied and analyzed by the method of Gaussian fit separation of the average profile (GFSAP). It has bee......
为探究吕家坨井田地质构造格局,根据钻孔勘探资料,采用分形理论和趋势面分析方法,研究了井田7......
Parkes脉冲星数据库目前已经收集了从1991年至今由Parkes望远镜观测的165755个数据文件.数据文件及其存取方法遵循虚拟天文台协议.......
Effects of dynamo magnetic fields on observational properties of accreting millisecond X-ray pulsars
In this paper,we have investigated accreting millisecond X-ray pulsars,which are rapidly rotating neutron stars in low-m......
脉冲星是一类自转极为稳定、辐射电磁脉冲的中子星。脉冲星研究的3个前沿领域使得与其相关的射电天文观测需要更多更宽的无线电频......
PSR J0742-2822 is known for its quasi-periodic changes in the observed pulse profile and spindown rate.In this paper,we ......
It is conjectured that coherent re-emission of cyclotron resonance absorption could result in pulsar giant pulses.This c......
毫秒脉冲星的自转频率非常稳定,提供了一种独立的基于遥远自然天体并能持续数百万乃至数十亿年的时间基准,具有稳定性强、运行时间......
本文考虑了天体的自引力,内部应力和内部运动对引力辐射的贡献,修正了M:Zimmermann给出的脉冲星Crab和Vela的数值表。......
利用蒙特卡洛方法，模拟了脉冲星磁球层中全极冠级联过程的非热辐射．对一给定的位于中子星表面以上一定高度的平行于开场线的电场，原初......
脉冲星的射电辐射与其他天体物理辐射源有很大的不同,因为它们有着极高的亮温度和高度的线或圆偏振.极高的亮温度意味着起作用的发......
详细介绍了脉冲星测时软件TEMPO2的应用算法和软件的使用方法。内容包括软件的下载、安装、各种程序接口的使用、数据模拟、软件的......
Parkes脉冲星数据库目前已经收集了从1991年至今由Parkes望远镜观测的165755个数据文件。数据文件及其存取方法遵循虚拟天文台协议......
We report here an investigation of the X-ray eclipse transitions of the high mass X-ray binary pulsar Cen X-3 in differe......
研究表明,与磁星模型相比较,反常X射线脉冲星的加速模型不能说明所观测到的自转周期的分布.为了解释熟知的最慢X射线脉冲星 2S 011......
搜寻射电脉冲星需要成熟的软件套路以保证有效地得到新发现。介绍了脉冲星搜寻过程，提供了安装脉冲星搜寻软件的工具，并给出了脉冲星......
本文利用欧洲脉冲星观测网（EPN）数据库里PSRB1259．63在1．52GHz、4．68GHz和8．28GHz三个频率上的线偏振位置角观测数据研究这颗脉冲星可能......
脉冲星自转的稳定性是其最显著的特征之一,利用这种特征可以提供脉冲星自身自转减慢的精确信息,研究强引力场中的广义相对论效应,......
费米γ射线空间望远镜(Fermi)自2008年8月观测任务开始以来,以其优越的观测性能开启了γ射线天文学研究的新纪元。其搭载的大面积......
努力被作理解预定行为(例如，在在 periastron 段落的投射脉冲星 semimajor 轴的 jumps ) 在 PSR B125963 的 13 年的监视观察了。像......
本文首先论述了决定脉冲星的演化参量和 B—P 图的意义,并用此参量绘出了脉冲星在 B—P 图上对于磁坊稳恒和衰减两种情况的不同演......
本文在前文研究的基础上对脉冲星磁倾角随年龄的演变做了深入研究。文中推出了适合用观测值计算的理论式子,并用它对四颗脉冲星磁......
针对X射线脉冲星导航在航天器轨道机动过程中精度不高甚至发散的问题,提出一种将X射线脉冲星导航结合惯性导航和紫外敏感器的组合......
本文研究了广义相对论效应和量子力学效应对中子量γ射线辐射的影响。通过选择磁偶极矩以及观察者视线与磁轴之间的夹角这两个观测......
According to two estimated relations between the initial period andthe dynamo-generated magnetic dipole field of pulsars......
According to two estimated relations between the initial period andthe dynamo-generated magnetic dipole field of pulsars......
基于把侧面划分成很多绝对阶段间隔，解决阶段的系列(PHRS ) 为经典 conal 在二十年在收音机频率从出版排列时间的平均侧面被导出 --......
我们再学习到宇宙的光线正电子的成熟 gamma 光线脉冲星的可能的贡献基于外部差距模型的新版本。在这个模型，倾斜角度和外部差距的......
The1S0nucleonic superfluids are investigated within the relativistic meanfield model and Bardeen-Cooper-Schrieffer theor......
Recently,the magnetar Swift J1834.9—0846 has been reported to have a possible wind nebula.It is shown that both the mag......
The glitch size,△ν/ν, inter-glitch time interval, ti, and frequency of glitches in pulsars are key parameters in disc......
Employing multiple pulsars and using an appropriate algorithm to establish ensemble pulsar timescale can reduce the infl......
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Fast Radio Bursts(FRBs) are intense radio flashes from the sky that are characterized by millisecond durations and Jansk......
Wide-bandwidth drift-scan pulsar surveys of globular clusters： application to early science observat
The Five-hundred-meter Aperture Spherical Telescope(FAST) will begin its early-science operations during 2016.Drift-scan......
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The observed recurrence of glitches in pulsars and neutron stars carries rich information about the evolution of their i......
