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- W2038589067 abstract "Although the majority of the discrete radio sources are unidentified, it is believed that they are very distant extragalactic objects. They may be galaxies with few visible stars. This paper examines physical conditions in large gas clouds, and shows that if these constitute the major class of radio sources a lower limit may be placed on their radio powers. If a large proportion of the mass is condensed into stars the conditions for gravitational stability, which form a part of the present argument, will not apply; however it appears that even under these circumstances the radio power must exceed 10 25 w. ster −1 (c/s) −1 at 80 Mc/s." @default.
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- W2038589067 date "1960-04-01" @default.
- W2038589067 modified "2023-10-09" @default.
- W2038589067 title "On the Dimensions, Spatial Density and Power of the Extragalactic Radio Sources" @default.
- W2038589067 doi "https://doi.org/10.1093/mnras/120.4.360" @default.
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