Highway Design and Construction 1988
DOI: 10.1007/978-1-349-10067-5_8
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“…However, only a few powerful radio galaxies have been imaged at these short wavelengths. Cygnus A, the brightest such object in the sky, has been observed with the Berkeley Illinois Maryland Association (BIMA) mm‐wave interferometer on several occasions (Wright & Birkinshaw 1984; Wright & Sault 1993) and with the Institut de Radioastronomie Millimétrique (IRAM) 30‐m telescope at 230 GHz (Salter et al 1989). Wright & Sault (1993) commented briefly on the global spectrum of the lobes of Cygnus A at ∼90 GHz, but their result does not tell us anything about the variation of the cm‐to‐mm spectrum of the source as a function of position.…”
Section: Introductionmentioning
confidence: 99%
“…However, only a few powerful radio galaxies have been imaged at these short wavelengths. Cygnus A, the brightest such object in the sky, has been observed with the Berkeley Illinois Maryland Association (BIMA) mm‐wave interferometer on several occasions (Wright & Birkinshaw 1984; Wright & Sault 1993) and with the Institut de Radioastronomie Millimétrique (IRAM) 30‐m telescope at 230 GHz (Salter et al 1989). Wright & Sault (1993) commented briefly on the global spectrum of the lobes of Cygnus A at ∼90 GHz, but their result does not tell us anything about the variation of the cm‐to‐mm spectrum of the source as a function of position.…”
Section: Introductionmentioning
confidence: 99%