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Chapter and Conference Paper
CO (1–0) Maps of NGC7027
NGC7027 is a very young planetary nebula in which the ionization of the red giant wind is only partially complete. Previous measurements of the CO (1–0) emission at 115 GHz from NGC7027 (Mufson, Lyon, Marioni,...
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Article
Very long baseline interferometry at a wavelength of 3.4 mm
In recent years the angular distribution of intensity of the compact cores of quasars and radio galaxies has been mapped in detail by very long baseline interferometry (VLBI) arrays1,2. These observations have sh...
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Article
Low-frequency variability and predicted superluminal motion in 3C147
VLBI observations of 3C147 reveal that its core is a low-frequency variable radio source which has brightened by a factor of 2 in 6 years. In combination with X-ray observations, this implies that bulk relativ...
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Chapter
Radio Astronomy
This report covers surveys of radio sources, basic measurements of source parameters and new developments in radio telescopes, instrumental techniques and data processing. The period covered is approximately l...
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Article
Radio sources with superluminal velocities
Radio data from four extragalactic sources, three quasars and one galaxy, show evidence for an apparent expansion faster than the speed of light. The data on these ‘superluminal’ sources are reviewed, and thei...
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Article
High resolution observations of NGC1275 with a four-element intercontinental radio interferometer
The radio nucleus of NGC1275 (3C84) is found to consist of three apparently stationary centres of emission extending over 0.006″ (3pc) along position angle −9°. One or more of these centres have changed their ...
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Article
Variations of Small Quasar Components at 2,300 MHz
IN a previous article1 we reported long-baseline interferometer measurements of several quasi-stellar radio sources using stations of the NASA/JPL Deep Space Network in Australia and California. Comparison of thr...
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Article
Trans-Pacific Interferometer Measurements at 2,300 MHz
Interferometer observations of ten radio sources, most of them quasars, with a baseline between California and Australia.
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Article
Further Observations of Pulsating Radio Sources at 13 cm
This article describes a series of measurements of the pulsating radio CP 0834, CP 0950, CP 1133 and CP 1919.
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Article
Detection of the Pulsed Radio Source CP 1919 at 13 cm Wavelength
High-frequency measurements suggest that the spectrum of the pulsating radio source is extremely steep.
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Chapter
Detection of the Pulsed Radio Source CP 1919 at 13 cm Wavelength
The pulsed radio source discovered at 3·68 m wavelength1 has been studied at various other wavelengths between 2 m and 73 cm2,3. The latter report states that the individual pulses have widths of about 35 ms with...
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Article
Distribution of Brightness in Extragalactic Radio Sources