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Measurements of general relativistic effects in the binary pulsar PSR1913 + 16
Measurements of second- and third-order relativistic effects in the orbit of binary pulsar PSR1913 + 16 have yielded self-consistent estimates of the masses of the pulsar and its companion,…
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Frequency dependence of the main pulse to interpulse separation for seven pulsars
In the course of a study of pulsar interpulses 43 bright pulsars were searched for interpulse emission. A previously undetected interpulse in PSR 1944 + 17 was found and improved upper limits were…
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Further observations of the binary pulsar PSR 1913+16.
We report the results of more than a year's timing observations of the binary pulsar PSR 1913+16. Within the accuracy of our measurements, about +- 300 ..mu..s, the pulse arrival times are exactly…
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Gravitational waves from an orbiting pulsar.
E instein's general theory of relativi­ ty, published in 1915, makes an extraordinary prediction: an ac­ celerating mass should radiate energy in the form of gravitational waves. Yet the waves are so…
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PSR 0031–07: The Harmonic Pulsar
In common with other older pulsars, the emission consists of long null stretches, occasionally interrupted by bursts of drifting sub­ pulses. The drifting subpulses always assume one of three…
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Inflationary Cosmology: Exploring the Universe from the Smallest to the Largest Scales
Pulsar flux observations: long-term intensity and spectral variations.
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Incremental Polarization of Starlight at Different Locations in the Galaxy
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Unusual properties of the pulsar PSR 1822-09
Mode-Changing, Drifting Subpulses, and Interpulse Emission in PSR 1822-09
PSR 1822-09 is a nearby galactic disk pulsar with a typical .769 s period. Its large period derivative indicates a young timing age of 250,000 yrs and a strong estimated surface magnetic field of…
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