Further observations of the binary pulsar PSR 1913+16
1976; IOP Publishing; Volume: 206; Linguagem: Inglês
10.1086/182131
ISSN1538-4357
AutoresJ. H. Taylor, R. Hülse, L. A. Fowler, G. E. Gullahorn, Joanna M. Rankin,
Tópico(s)Inertial Sensor and Navigation
Resumoview Abstract Citations (117) References (15) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Further observations of the binary pulsar PSR 1913+16. Taylor, J. H. ; Hulse, R. A. ; Fowler, L. A. ; Gullahorn, G. E. ; Rankin, J. M. Abstract Results are reported for more than a year's timing observations of the binary pulsar PSR 1913+16. Within the accuracy of the measurements, the pulse arrival times are exactly those expected from a clock of well-defined period moving in a Keplerian orbit with a constant rate of apsidal advance. The observations have yielded much-improved values for the parameters of the pulsar and its orbit, and are approaching the length of baseline needed to perform certain tests of gravitation theories. An upper limit of 60 microjansky is placed on periodically pulsed radio emission from the companion object. Publication: The Astrophysical Journal Pub Date: May 1976 DOI: 10.1086/182131 Bibcode: 1976ApJ...206L..53T Keywords: Binary Stars; Orbit Calculation; Periodic Variations; Pulsars; Companion Stars; Long Term Effects; Radio Emission; Stellar Mass; Astronomy full text sources ADS | data products SIMBAD (1)
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