A survey of the radio continuum emission of RS Canum Venaticorum and related active binary systems

Details A survey of the radio continuum emission of RS Canum Venaticorum and related active binary systems A survey of the radio continuum emission of RS Canum Venaticorum and related active binary systems

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apjs...71..905d&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 71, Dec. 1989, p. 905-930.

Astronomy and Astrophysics

Astronomy

134

Binary Stars, Continuous Radiation, Radio Emission, Sky Surveys (Astronomy), Starspots, Stellar Coronas, Stellar Luminosity, Stellar Rotation, Ultraviolet Radiation, Very Large Array (Vla), X Ray Spectra

Scientific paper

Observations of 77 RS CVn and related active binary systems were made with VLA at a continuum frequency of 4.86 GHz. The results are combined with other VLA observations to produce a total number of observed sources of 122. A search for correlations of radio properties with various systemic and stellar parameters is performed. Significant correlations are found between the normalized radio luminosity L(6)/L(bol) and the normalized soft X-ray luminosity L(x)/L(bol). It is suggested that the close correlation between low-level 6-cm emission and the hot component of the soft X-ray emission observed by the Einstein solid state spectrometer is caused by both emissions being produced by the same thermal electrons.

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