The Thousand-Pulsar-Array programme on MeerKAT - XVII. Discovery of beating radio emission variability in PSR J1514-4834

被引:0
|
作者
Hsu, J. A. [1 ]
Weltevrede, P. [1 ]
Wright, G. [1 ]
Keith, M. J. [1 ]
Oswald, L. S. [2 ]
Song, X. [3 ]
Wang, H. [1 ]
机构
[1] Univ Manchester, Jodrell Bank Ctr Astrophys, Dept Phys & Astron, Manchester M13 9PL, England
[2] Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, England
[3] Netherlands Inst Radio Astron, ASTRON, Oude Hoogeveensedijk 4, NL-7991 PD Dwingeloo, Netherlands
基金
新加坡国家研究基金会; 英国科学技术设施理事会;
关键词
pulsars: general; pulsars: individual: J1514-4834; DRIFTING SUBPULSES; FREQUENCY-DEPENDENCE; EMPIRICAL-THEORY; PERIODIC NULLS; MODULATION; POLARIZATION; B0943+10; MODE; BEHAVIOR; TOPOLOGY;
D O I
10.1093/mnras/staf323
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a comprehensive analysis of the complex subpulse modulation patterns in PSR J1514-4834 (B1510-48) using L-band data from the Thousand-Pulsar-Array (TPA) programme, complemented with further MeerKAT UHF-band data. We demonstrate that periodic drifting subpulses and rapid amplitude modulation with a period of about two pulse periods co-exist. It is established that these two periodic emission patterns interfere in the form of a beat system, giving rise to multiple spectral features. We develop a new methodology which confirms the expected correlations in the complex phase of the beat features in a two-dimensional Fourier transform of the data. Therefore, a relatively simple beat system can explain the complex single-pulse behaviour of this pulsar. The simultaneous coexistence of multiple subpulse modulation periodicities is rare in the population and points to poorly understood intricate dynamics within pulsar magnetospheres. A comparison with PSR B0943+10 is made, for which the coexistence of multiple periodicities has been argued to be a natural consequence of a rotating carousel. However, our observations of PSR J1514-4834 require a different explanation, involving time-delayed interactions between separate regions of the magnetosphere. The developed phase correlation methodology opens up the route for underlying beat systems in the modulation patterns of more pulsars.
引用
收藏
页码:1063 / 1080
页数:18
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