Extragalactic Radio Continuum
Extragalactic Radio Continuum is a non-thermal electromagnetic emission phenomenon in the radio frequency range originating from astrophysical sources outside the Milky Way Galaxy, distinguished by its diffuse synchrotron radiation mechanisms and absence of discrete spectral lines.
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751
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Publications per year
2017–2026
117
Parents
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A superluminal source in the Galaxy
I. F. Mirabel, Luis F. Rodrı́guez · Nature · 1994 · 1.2K citations
A bright millisecond-duration radio burst from a Galactic magnetar
Nature · 2020 · 718 citations · Full text
Natural Sciences, Astronomy, Physics +12
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Commonwealth Scientific and Industrial Research Organisation, Australia
19 publications · 1.2K citations
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National Radio Astronomy Observatory
Charlottesville, United States
56 h-index
260 publications
19.1K citations
Max Planck Institute for Radio Astronomy
Bonn, Germany
48 h-index
287 publications
18K citations

Commonwealth Scientific and Industrial Research Organisation
Canberra, Australia
40 h-index
186 publications
14.3K citations
California Institute of Technology
Pasadena, United States
39 h-index
151 publications
16.3K citations
Istituto di Radioastronomia di Bologna
Bologna, Italy
36 h-index
123 publications
6.4K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
35 h-index
95 publications
4.2K citations
Netherlands Institute for Radio Astronomy
Dwingeloo, The Netherlands
34 h-index
83 publications
4.7K citations
Australia Telescope National Facility
Sydney, Australia
32 h-index
116 publications
8.4K citations
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ApJ · 383 publications · 19.8K citations
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189 publications · 9.4K citations
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131 publications · 7.2K citations
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AJ · 120 publications · 5.4K citations
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74 publications · 7.3K citations
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