Published 1994
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Timing Observations of the SMC Binary PSR J0045-7319
Chicago
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.
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© 1994 International Astronomical Union • Provided by the NASA Astrophysics Data System.Attached Files
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Additional details
- Eprint ID
- 67796
- Resolver ID
- CaltechAUTHORS:20160608-203753832
- Created
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2016-06-09Created from EPrint's datestamp field
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2020-03-09Created from EPrint's last_modified field
- Caltech groups
- Owens Valley Radio Observatory, Infrared Processing and Analysis Center (IPAC)
- Series Name
- IAU Symposium Proceedings Series
- Series Volume or Issue Number
- 165