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Discovery of a 24 ms Pulsar in a Very Long Orbit with the Murchison Widefield Array

  • Authors: Chia Min Tan, N. D. Ramesh Bhat, Bradley W. Meyers, Christopher P. Lee, Ewan D. Barr, Vivek Venkatraman Krishnan, Paulo C. C. Freire, Garvit Grover, Samuel J. McSweeney, Nicholas A. Swainston, Qiuyang Fu, Mengyao Xue

Chia Min Tan et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 9.

Scatter plot showing the eccentricity and the minimum companion mass of the 16 pulsars with known binary orbital periods of more than 290 days. The circle points are companions that are most likely to be main-sequence stars, and the triangle points are companions that are most likely to be white dwarfs. PSR J0125−5854 is shown as a cross. The color of the points shows the spin period of the pulsars in their respective binary system.

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