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- W2000306356 abstract "The radio source 4C 11.50 is double at 365 MHz and at 2695 MHz; at the latter frequency one component agrees in position with the brighter of the close pair of QSOs studied by Wampler et al . At 8085 MHz, only one component was observed, and its position again agrees with that of the brighter QSO. An upper limit of 0.05 × 10 −26 W m −2 Hz −1 at 2695 and 8085 MHz can be set to emission from the fainter QSO or from the red galaxy about 10″ arc away from the brighter QSO." @default.
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- W2000306356 date "1974-04-01" @default.
- W2000306356 modified "2023-09-25" @default.
- W2000306356 title "Radio Observations of the 'Double QSO' 4C 11.50" @default.
- W2000306356 doi "https://doi.org/10.1093/mnras/167.1.75p" @default.
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