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

ABSTRACT 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.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2025-02-20
DOI
https://doi.org/10.1093/mnras/staf323
Citations
3
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
3.46

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article

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

L S Oswald, P. Weltevrede, X Song, J A Hsu et al.
3 citations
Monthly Notices of the Royal Astronomical Society
Pulsars and Gravitational Waves Research
3.46
article

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

L S Oswald, P. Weltevrede, X Song, J A Hsu, M. J. Keith, G. A. E. Wright, Huabing Wang
article en
3 citations

Abstract

ABSTRACT 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.

Monthly Notices of the Royal Astronomical SocietyVol. 538(2)
University of Manchester (GB), AstroTec Holding (Netherlands) (NL), University of Southampton (GB), Netherlands Institute for Radio Astronomy (NL)
National Research Foundation, Swinburne University of Technology, Science and Technology Facilities Council
Openalex Percentile: Top 9%
Pulsars and Gravitational Waves Research
3.46
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