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The thousand-pulsar-array programme on MeerKAT – XVII. Discovery of beating radio emission variability in PSR J1514−4834

The thousand-pulsar-array programme on MeerKAT – XVII. Discovery of beating radio emission variability in PSR J1514−4834
The thousand-pulsar-array programme on MeerKAT – XVII. Discovery of beating radio emission variability in PSR J1514−4834
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.
astro-ph.HE, pulsars: general, pulsars: individual: J1514–4834
1365-2966
1063-1080
Hsu, J.A.
2776a280-4444-437e-ba69-97140241a584
Weltevrede, P.
cf899f41-558f-4425-8685-3defdab81444
Wright, G.
9828a681-5c69-4917-b7c7-0434ece56bda
Keith, M.J.
cc80da04-048c-45e3-9e58-c51311630107
Oswald, L.S.
37bd35fc-2e68-4a79-8ada-fefaa61fa959
Song, X.
281a067d-3e5a-4c3e-9be5-8174e0d9d440
Wang, H.
b09cec25-b668-4f1f-96fa-f6bb2c49abbc
Hsu, J.A.
2776a280-4444-437e-ba69-97140241a584
Weltevrede, P.
cf899f41-558f-4425-8685-3defdab81444
Wright, G.
9828a681-5c69-4917-b7c7-0434ece56bda
Keith, M.J.
cc80da04-048c-45e3-9e58-c51311630107
Oswald, L.S.
37bd35fc-2e68-4a79-8ada-fefaa61fa959
Song, X.
281a067d-3e5a-4c3e-9be5-8174e0d9d440
Wang, H.
b09cec25-b668-4f1f-96fa-f6bb2c49abbc

Hsu, J.A., Weltevrede, P., Wright, G., Keith, M.J., Oswald, L.S., Song, X. and Wang, H. (2025) The thousand-pulsar-array programme on MeerKAT – XVII. Discovery of beating radio emission variability in PSR J1514−4834. Monthly Notices Of The Royal Astronomical Society, 538 (2), 1063-1080. (doi:10.1093/mnras/staf323).

Record type: Article

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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Accepted/In Press date: 20 February 2025
e-pub ahead of print date: 21 February 2025
Published date: 12 March 2025
Keywords: astro-ph.HE, pulsars: general, pulsars: individual: J1514–4834

Identifiers

Local EPrints ID: 501133
URI: http://eprints.soton.ac.uk/id/eprint/501133
ISSN: 1365-2966
PURE UUID: 3e1850a4-cc2d-4bc2-beda-b7a0d4304ea7
ORCID for L.S. Oswald: ORCID iD orcid.org/0000-0002-0838-0680

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Date deposited: 27 May 2025 16:38
Last modified: 03 Sep 2025 02:12

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Contributors

Author: J.A. Hsu
Author: P. Weltevrede
Author: G. Wright
Author: M.J. Keith
Author: L.S. Oswald ORCID iD
Author: X. Song
Author: H. Wang

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