A search for radio emission from late-type supergiant stars

Details A search for radio emission from late-type supergiant stars A search for radio emission from late-type supergiant stars

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....60..277s&link_type=abstract

Astronomy and Astrophysics, vol. 60, no. 2, Sept. 1977, p. 277-280.

Astronomy and Astrophysics

Astronomy

18

Late Stars, Microwave Emission, Radio Astronomy, Stellar Radiation, Supergiant Stars, Radio Stars, Stellar Luminosity, Variable Stars

Scientific paper

Radio continuum observations at 10.5 GHz have been made of 29 high-luminosity F0-K5 supergiant stars. Two sources were detected (at the 3-sigma confidence level) in this survey. One corresponds to the unusual spectrum-variable star HR 8752=HD 217476 (G0 Ia). The other is located approximately one arc minute southwest of the star HD 18391 (G0 Ia), with a positional error box containing no obvious optical candidate(s).

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