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- W1979785812 abstract "Previous observations of Cep A have shown the presence of a highly variable source 8. During subsequent monitoring over the period 1988 November 2 to 1990 May 8, a second new highly variable radio source has appeared. The latter is more isolated from the other more diffuse regions, and thus accurate measurements of spectra been possible at 1.5 × 10 9 , 5.0 × 10 9 and 1.5 × 10 10 Hz. A number of possible mechanisms for the origin of the radiation from both sources is discussed, but the resulting interpretation of the spectra is in terms of gyrosynchrotron emission from thermal electrons at a temperature ∼ 10 8 K, in magnetic field ∼ 200 G, and a region of size ∼ 1 AU." @default.
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- W1979785812 date "1991-12-01" @default.
- W1979785812 modified "2023-09-27" @default.
- W1979785812 title "Time-dependent radio sources in the star-forming region Cepheus A (east)" @default.
- W1979785812 doi "https://doi.org/10.1086/170784" @default.
- W1979785812 hasPublicationYear "1991" @default.
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