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Periodic interstellar scintillation variations of PSRs J0613–0200 and J0636+5128 associated with the Local Bubble shell

Liu, Yulan; Main, Robert A.; Verbiest, Joris P.W.; Wu, Ziwei; Ambalappat, Krishnakumar M.; Lu, Jiguang; Champion, David J.; Cognard, Ismaël; Guillemot, Lucas; Liu, Kuo; McKee, James W.; Porayko, Nataliya; Shaifullah, Golam M.; Theureau, Gilles

Authors

Yulan Liu

Robert A. Main

Joris P.W. Verbiest

Ziwei Wu

Krishnakumar M. Ambalappat

Jiguang Lu

David J. Champion

Ismaël Cognard

Lucas Guillemot

Kuo Liu

James W. McKee

Nataliya Porayko

Golam M. Shaifullah

Gilles Theureau



Abstract

Annual variations of interstellar scintillation can be modelled to constrain parameters of the ionized interstellar medium. If a pulsar is in a binary system, then investigating the orbital parameters is possible through analysis of the orbital variation of scintillation. In observations carried out from 2011 to 2020 by the European Pulsar Timing Array radio telescopes, PSRs J0613–0200 and J0636+5128 show strong annual variations in their scintillation velocity, while the former additionally exhibits an orbital fluctuation. Bayesian theory and Markov-chain-Monte-Carlo methods are used to interpret these periodic variations. We assume a thin and anisotropic scattering screen model, and discuss the mildly and extremely anisotropic scattering cases. PSR J0613–0200 is best described by mildly anisotropic scattering, while PSR J0636+5128 exhibits extremely anisotropic scattering. We measure the distance, velocity, and degree of anisotropy of the scattering screen for our two pulsars, finding that scattering screen distances from Earth for PSRs J0613–0200 and J0636+5128 are 316 −20+28 pc and 262 −38+96 pc, respectively. The positions of these scattering screens are coincident with the shell of the Local Bubble towards both pulsars. These associations add to the growing evidence of the Local Bubble shell as a dominant region of scattering along many sightlines.

Citation

Liu, Y., Main, R. A., Verbiest, J. P., Wu, Z., Ambalappat, K. M., Lu, J., Champion, D. J., Cognard, I., Guillemot, L., Liu, K., McKee, J. W., Porayko, N., Shaifullah, G. M., & Theureau, G. (2023). Periodic interstellar scintillation variations of PSRs J0613–0200 and J0636+5128 associated with the Local Bubble shell. Science China Physics, Mechanics and Astronomy, 66(11), Article 119512. https://doi.org/10.1007/s11433-023-2182-6

Journal Article Type Article
Acceptance Date Jul 19, 2023
Online Publication Date Oct 10, 2023
Publication Date Nov 1, 2023
Deposit Date Oct 26, 2023
Publicly Available Date Nov 28, 2024
Journal Science China: Physics, Mechanics and Astronomy
Print ISSN 1674-7348
Electronic ISSN 1869-1927
Publisher Chinese Academy of Sciences
Peer Reviewed Peer Reviewed
Volume 66
Issue 11
Article Number 119512
DOI https://doi.org/10.1007/s11433-023-2182-6
Keywords Pulsar; Interstellar scintillation; Ionized interstellar medium
Public URL https://hull-repository.worktribe.com/output/4426014
Other Repo URL https://arxiv.org/abs/2307.09745

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Copyright Statement
© Science China Press and Springer-Verlag Berlin Heidelberg 2017

This version of the article has been accepted for publication, after peer review (when applicable) and is subject to Springer Nature’s AM terms of use, but is not the Version of Record and does not reflect post-acceptance improvements, or any corrections.





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