Radio Lobes
Radio Lobe is a large-scale, magnetized region of relativistic plasma extending outward from the central galaxy in an active galactic nucleus, distinct from other emission structures by its diffuse, lobe-shaped morphology and synchrotron radiation origin, typically observed at radio wavelengths and fed by jets emanating from the central supermassive black hole.
582
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33.1K
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1.6K
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501
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2017–2026
69
582
Chandra imaging of the complex X-ray core of the Perseus cluster
A. C. Fabian, J. S. Sanders, S. Ettori et al. · Monthly Notices of the Royal Astronomical Society · 2000 · 627 citations · Full text
Natural Sciences, Astronomy, Physics +14
Overpressured cocoons in extragalactic radio sources
Mitchell C. Begelman, Denis F. Cioffi · The Astrophysical Journal · 1989 · 503 citations
Natural Sciences, Astronomy, Physics +16
Appearance of Relativistically Expanding Radio Sources
M. J. Rees · Nature · 1966 · 488 citations
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501
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
35 h-index
168 publications
13.6K citations
National Radio Astronomy Observatory
Charlottesville, United States
32 h-index
72 publications
4.8K citations
University of Hertfordshire
Hatfield, United Kingdom
28 h-index
60 publications
3.7K citations
Istituto di Radioastronomia di Bologna
Bologna, Italy
28 h-index
105 publications
4K citations

Commonwealth Scientific and Industrial Research Organisation
Canberra, Australia
27 h-index
85 publications
3.6K citations
Netherlands Institute for Radio Astronomy
Dwingeloo, The Netherlands
23 h-index
117 publications
7.3K citations

University of Bologna
Bologna, Italy
21 h-index
52 publications
2.8K citations
National Centre for Radio Astrophysics
Pune, India
20 h-index
48 publications
1.5K citations
1–8 of 501
ApJ · 202 publications · 13.1K citations
61
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153 publications · 8.7K citations
49
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52 publications · 2.2K citations
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AJ · 30 publications · 1.2K citations
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22 publications · 2.2K citations
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