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Observation of the quasar 3C47 with the interferometer URAN at decametric wavelengths

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Abstract

Preliminary results of the observation of the angular structure of the quasar 3C47 at 20 and 25 MHz using the URAN-1 interferometer are presented. The most probable model of the brightness distribution of this source at decameter wavelengths has been determined. This model consists of two extended components having angular dimensions about 22 arcsec and separated by about 50 arcsec.

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Authors
  1. A. V. Men'
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  2. S. Ya. Braude
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  3. S. L. Rashkovsky
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  4. N. K. Sharykin
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  5. V. A. Shepelev
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  6. G. A. Inyutin
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  7. A. D. Khristenko
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  8. G. S. Podgorny
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Additional information

Radioastronomical Institute, Ukrainian Academy of Sciences, Khar'kov. Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 38, No. 6, pp. 511–521, June, 1995.

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Men', A.V., Braude, S.Y., Rashkovsky, S.L. et al. Observation of the quasar 3C47 with the interferometer URAN at decametric wavelengths. Radiophys Quantum Electron 38, 336–343 (1995). https://doi.org/10.1007/BF01037766

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  • DOI: https://doi.org/10.1007/BF01037766

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