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• W2502970340 abstract "Compact radio stars are associated with both galaxies and quasi-stellar objects; and there appears to be no way to distinguish between the radio galaxies and the quasi-stellar radio sources from their radio properties alone. The compact radio sources are opaque at the longer radio wavelengths and have spectra that are either peaked or complex. They have a complex brightness distribution and often contain components less than 0.001 arc sec in size. Many of the compact sources show large intensity variations and in NGC 1275 there is evidence for a change in the angular size during one year." @default.
• W2502970340 created "2016-08-23" @default.
• W2502970340 creator A5066709362 @default.
• W2502970340 date "1972-01-01" @default.
• W2502970340 modified "2023-09-26" @default.
• W2502970340 title "Radio Emission from Compact Objects" @default.
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• W2502970340 doi "https://doi.org/10.1017/s0074180900005520" @default.
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