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The polarization characteristics of the radio emission of the pulsars CP 0950 and CP 1133 at the 3.5 m wavelength

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Radiophysics and Quantum Electronics Aims and scope

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Literature Cited

  1. Yu. I. Alekseev, S. M. Kutuzov, M. M. Tyaptin, and V. D. Chuikov, Transactions of the Physics Institute [in Russian], Izd. AN SSSR, Vol. 62 (1972), p. 121.

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  2. H. D. Graft, Jr. and J. M. Comella, Nature,220, 676 (1968).

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  3. V. V. Vitkevich, V. M. Malofeev, and Yu. I. Alekseev, Dokl. Akad. Nauk SSSR,205, 307 (1972).

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Authors
  1. Yu. I. Alekseev
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Additional information

P. N. Lebedev Physics Institute, Academy of Sciences of the USSR. Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 16, No. 5, pp. 762–764, May, 1973.

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Alekseev, Y.I. The polarization characteristics of the radio emission of the pulsars CP 0950 and CP 1133 at the 3.5 m wavelength. Radiophys Quantum Electron 16, 585–587 (1973). https://doi.org/10.1007/BF01033496

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  • DOI: https://doi.org/10.1007/BF01033496

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