stars:neutron相关论文
So far quite a few ultraluminous X-ray (ULX) pulsars have been discovered.In this work,we construct a super-Eddington,ma......
The single pulse observation of PSR J1752+2359 at 1250 MHz made using the Five-hundred-meter Aperture Spherical radio Te......
PSR J1946 + 3417 is a millisecond pulsar (MSP) with a spin period P ≈ 3.17 ms.Harbored in a binary with an orbital peri......
So far quite a few ultraluminous X-ray(ULX) pulsars have been discovered.In this work,we construct a super-Eddington,mag......
Pulsar timing is a classic technology of detecting irregularities in pulsar rotation.We carried out this method for 18 y......
The LOw-Frequency ARray (LOFAR) has recently conducted a survey (LOFAR Tied-Array All-sky Survey;LOTAAS) for pulsars in ......
We investigated the pulsar radio luminosity(L),emission efficiency(ratio of radio luminosity to its spin-down power E),a......
Several X-ray binaries (XRBs) have been identified to be associated with supernova remnants(SNRs). Because of the short ......
The accretion-induced collapse(AIC)scenario was proposed 40 years ago as an evolutionary end state of oxygen-neon white ......
Recently,a 16-day periodicity in a fast radio burst was reported.We propose that this 16-day periodicity may be due to f......
Resonant cyclotron scattering in pulsar magnetospheres and its application to isolated neutron stars
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......
The LOw-Frequency ARray(LOFAR)has recently conducted a survey(LOFAR Tied-Array Allsky Survey;LOTAAS)for pulsars in the N......
The form of timing residuals due to errors in pulsar spin period P and its derivative P, in positions, as well as in pro......
One large glitch was detected in PSR B1737-30 using data spanning from MJD 57999 to 58406 obtained with the newly built ......
Revisiting the event rate of short GRBs and estimating their detectable number within the Advanced L
The redshift and luminosity distributions of 36 Swift short gamma-ray bursts(GRBs) are fitted by connecting their event ......
We consider the existence of a neutron star magnetic field by the detected cyclotron lines. We collected data on nine so......
We report on the first analysis of an AstroSat observation of the Z-source GX 5–1 on 2017 February 26-27. The hardness-......
Accreting millisecond X-ray pulsars(AMXPs) are an important subclass of low-mass X-ray binaries(LMXBs), in which coheren......
With the constraint from gravitational wave emission of a binary merger system(GW170817)and two-solar-mass pulsar observ......
I present a novel mechanism to boost magnetic field amplification of newly born neutron stars in core collapse supernova......
