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<p>The ionized interstellar medium contains astronomical-unit-scale (and below) structures that scatter radio waves from pulsars, resulting in scintillation. Power spectral analysis of scintillation often shows parabolic arcs, with curvatures that encode the locations and kinematics of the pulsar, Earth and interstellar plasma. Here we report the discovery of 25 distinct plasma structures in the direction of the brilliant millisecond pulsar, PSR J0437−4715, in observations obtained with the MeerKAT radio telescope. Four arcs reveal structures within 5,000 au of the pulsar, from a series of shocks induced as the pulsar and its wind interact with the ambient interstellar medium. The measured radial distance and velocity of the main shock allow us to solve the shock geometry and space velocity of the pulsar in three dimensions, whereas the velocity of another structure unexpectedly indicates a back flow from the direction of the shock or pulsar-wind tail. The remaining 21 arcs represent a surprising abundance of structures sustained by turbulence within the Local Bubble, which is a region of the interstellar medium thought to be depleted of gas by a series of supernova explosions about 14 Myr ago. The Local Bubble is cool enough in areas for subastronomical-unit density fluctuations to arise from turbulence.</p>

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Bow shock and Local Bubble plasma unveiled by the scintillating millisecond pulsar J0437−4715

  • 期刊论文

  • 发表日期：

    2025年4月21日

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  • Daniel J. Reardon,
  • Robert Main,
  • Stella Koch Ocker,
  • Ryan M. Shannon,
  • Matthew Bailes,
  • Fernando Camilo,
  • Marisa Geyer,
  • Andrew Jameson,
  • Michael Kramer,
  • Aditya Parthasarathy,
  • Renée Spiewak,
  • Willem van Straten,
  • Vivek Venkatraman Krishnan

摘要

The ionized interstellar medium contains astronomical-unit-scale (and below) structures that scatter radio waves from pulsars, resulting in scintillation. Power spectral analysis of scintillation often shows parabolic arcs, with curvatures that encode the locations and kinematics of the pulsar, Earth and interstellar plasma. Here we report the discovery of 25 distinct plasma structures in the direction of the brilliant millisecond pulsar, PSR J0437−4715, in observations obtained with the MeerKAT radio telescope. Four arcs reveal structures within 5,000 au of the pulsar, from a series of shocks induced as the pulsar and its wind interact with the ambient interstellar medium. The measured radial distance and velocity of the main shock allow us to solve the shock geometry and space velocity of the pulsar in three dimensions, whereas the velocity of another structure unexpectedly indicates a back flow from the direction of the shock or pulsar-wind tail. The remaining 21 arcs represent a surprising abundance of structures sustained by turbulence within the Local Bubble, which is a region of the interstellar medium thought to be depleted of gas by a series of supernova explosions about 14 Myr ago. The Local Bubble is cool enough in areas for subastronomical-unit density fluctuations to arise from turbulence.