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Published 1994 | Published
Book Section - Chapter Open

Timing Observations of the SMC Binary PSR J0045-7319

Abstract

We describe radio timing observations of the binary pulsar PSR J0045-7319 made over the past 3.3 yr. We show that a simple timing model involving a standard Keplerian orbit well-describes the data, however significant lowlevel systematic residuals never before seen in other binary pulsars remain. We consider various possible origins of the residuals.

Additional Information

© 1994 International Astronomical Union • Provided by the NASA Astrophysics Data System.

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Created:
August 20, 2023
Modified:
January 13, 2024