Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 7.

Top: the solid line shows the variation of the spin period expected from the best-fit orbital model for the PSR J0125−5854 system, and the blue dots show the measured periods of the pulsar at all observation epochs. Bottom: the residuals in the measured spin periods compared to the expected values from the modeled orbit. The rms value and the reduced χ2 of the fit are 5 × 10−6 ms and 7.3, respectively.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse