Titlebook: Galactic and Extra-Galactic Radio Astronomy; Gerrit L. Verschuur,Kenneth I. Kellermann Book 19741st edition Springer-Verlag New York Inc.

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Galactic Nonthermal Continuum Emission,d through some process occurring at the subsolar point. These inferences were sharply revised when, after an entire year of observation, it was noted that the direction to the disturbance was not correlated with the position of the Sun, that it rather referred to afixed direction in space. Jansky (1

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The Radio Characteristics of HII Regions and the Diffuse Thermal Background,s. Because it is hotter than the surrounding medium, the gas of planetary and bright diffuse nebulae as well as supernova remnants emits spectral lines which appear in emission. These nebulae are categorically known as ..

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Pulsars,the Molonglo Radio Observatory in Australia, where about 30 of the presently known pulsars have been discovered. Pulsars were not discovered earlier because in most radio astronomical observations, receivers have relatively long time constants to smooth out random noise fluctuations. Consequently th

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The Galactic Magnetic Field, medium, which contains both thermal electrons and magnetic fields, can be decomposed into two oppositely circularly polarized components having different phase velocities. On emergence from the medium the waves can be recombined, but with relative phases which may be different from those which they

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Ernest H. Y. Chu,Sandra S. Powells. Because it is hotter than the surrounding medium, the gas of planetary and bright diffuse nebulae as well as supernova remnants emits spectral lines which appear in emission. These nebulae are categorically known as ..

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