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Radio Stars Beta Persei and Beta Lyrae

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Abstract

FOLLOWING the discovery that the radio emission of the Antares system originates from the B3 V component1,2, observations of other binary star systems were undertaken with the NRAO interferometer operating at 2,695 and 8,085 MHz. Here we report the detection of radio emission from two well known eclipsing binaries, β Persei (Algol) and β Lyrae.

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Authors and Affiliations

  1. National Radio Astronomy Observatory, Green Bank, West Virginia

    C. M. WADE & R. M. HJELLMING

Authors
  1. C. M. WADE
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  2. R. M. HJELLMING
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WADE, C., HJELLMING, R. Radio Stars Beta Persei and Beta Lyrae. Nature 235, 270–271 (1972). https://doi.org/10.1038/235270a0

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  • DOI: https://doi.org/10.1038/235270a0

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