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Detection of quasi-periodic micro-structure in three millisecond pulsars with the Large European Array for Pulsars

Liu, K.; Antoniadis, J.; Bassa, C. G.; Chen, S.; Cognard, I.; Gaikwad, M.; Hu, H.; Jang, J.; Janssen, G. H.; Karuppusamy, R.; Kramer, M.; Lee, K. J.; Main, R. A.; Mall, G.; Mckee, J. W.; Mickaliger, M. B.; Perrodin, D.; Sanidas, S. A.; Stappers, B. W.; Wang, L.; Zhu, W. W.; Burgay, M.; Concu, R.; Corongiu, A.; Melis, A.; Pilia, M.; Possenti, A.

Authors

K. Liu

J. Antoniadis

C. G. Bassa

S. Chen

I. Cognard

M. Gaikwad

H. Hu

J. Jang

G. H. Janssen

R. Karuppusamy

M. Kramer

K. J. Lee

R. A. Main

G. Mall

M. B. Mickaliger

D. Perrodin

S. A. Sanidas

B. W. Stappers

L. Wang

W. W. Zhu

M. Burgay

R. Concu

A. Corongiu

A. Melis

M. Pilia

A. Possenti



Abstract

We report on the detection of quasi-periodic micro-structure in three millisecond pulsars (MSPs), PSRs J1022+1001, J2145-0750, and J1744-1134, using high time resolution data acquired with the Large European Array for Pulsars at a radio frequency of 1.4 GHz. The occurrence rate of quasi-periodic micro-structure is consistent among pulses with different peak flux densities. Using an auto-correlation analysis, we measure the periodicity and width of the micro-structure in these three pulsars. The detected micro-structure from PSRs J1022+1001 and J1744-1134 is often highly linearly polarized. In PSR J1022+1001, the linear polarization position angles of micro-structure pulses are in general flat with a small degree of variation. Using these results, we further examine the frequency and rotational period dependency of micro-structure properties established in previous work, along with the angular beaming and temporal modulation models that explain the appearance of micro-structure. We also discuss a possible link of micro-structure to the properties of some of the recently discovered fast radio bursts which exhibit a very similar emission morphology.

Citation

Liu, K., Antoniadis, J., Bassa, C. G., Chen, S., Cognard, I., Gaikwad, M., …Possenti, A. (2022). Detection of quasi-periodic micro-structure in three millisecond pulsars with the Large European Array for Pulsars. Monthly notices of the Royal Astronomical Society, 513(3), 4037-4044. https://doi.org/10.1093/mnras/stac1082

Journal Article Type Article
Acceptance Date Apr 13, 2022
Online Publication Date Apr 27, 2022
Publication Date Jul 1, 2022
Deposit Date Nov 29, 2022
Publicly Available Date Dec 14, 2022
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 513
Issue 3
Pages 4037-4044
DOI https://doi.org/10.1093/mnras/stac1082
Keywords Methods: data analysis; Pulsars: individual (PSR J1022+1001); Pulsars: individual (PSR J2145−0750); Pulsars: individual (PSR J1744−1134); (transients:) fast radio bursts
Public URL https://hull-repository.worktribe.com/output/4134730

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Publisher Licence URL
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Copyright Statement
© 2022 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.




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