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Continuum Radio Emission from the Vicinity of Pulsars
Nature Physical Science, 1973Blandford et al.1 suggest the possibility of the existence of weak radio haloes around old pulsars. They attempt to explain the peculiar non-thermal shell source near PSR1919 + 21 (refs. 2–4) and suggest observations of the surroundings of pulsars to be carried out.
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Properties of the Radio Continuum Emission from Interacting Galaxies
Nature, 1973SEVERAL interacting galaxies have been observed recently in different programmes using the Westerbork Synthesis Radio Telescope at 21 cm wavelength (beamwidth 24 s × 24 s cosec δ). We give here a compilation of the data in order to examine the morphology, strength, and the frequency of occurrence of the radio emission from these interacting systems.
R. J. ALLEN +3 more
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Splotless flares and the associted radio continuum emission
Solar physics, 1987.
Ruždjak, Vladimir, Vršnak, Bojan
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Decimeter Continuum Radio Emission from a Post-Flare Loop
Solar Physics, 1986Radio observations offer an important means for providing estimates of magnetic fields in post-flare loops.
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Water Masers and Radio Continuum Emission Tracing Thermal Radio Jets
2009We present interferometric observations of radio continuum and water maser emission carried out with the Very Large Array (VLA1) toward five massive star-forming regions. Radio continuum sources were detected toward all star-forming regions and some of them could be thermal radio jets. In addition, although water maser emission was found in all massive
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Radio continuum and OH line emission of high-z OH megamaser galaxies
Astronomy and Astrophysics, 2023Yulia Sotnikova, Chun Sun
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Evolution of thermal and non-thermal radio continuum emission on kpc scales – predictions for SKA
Monthly Notices of the Royal Astronomical Society, 2022Masoumeh Ghasemi-Nodehi +2 more
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The Large-Scale Radio Continuum Emission of Spiral Galaxies
1990In this paper I review the recent results on the radio continuum emission from spiral galaxies. The emphasize is on the large-scale non-thermal emission which arises from the interaction between cosmic ray electrons and magnetic fields.
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Anisotropic Optical Continuum Emission in Radio Quasars
1994J. C. Baker +3 more
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