Radio emission from the RS Canum Venaticorum binary RT Lacertae

Details Radio emission from the RS Canum Venaticorum binary RT Lacertae Radio emission from the RS Canum Venaticorum binary RT Lacertae

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pasp...90..751g&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 90, Dec. 1978-Jan. 1979, p. 751-753.

Other

11

Binary Stars, Radio Stars, Variable Stars, White Dwarf Stars, Interferometry, Low Frequencies, Nonthermal Radiation, Radio Bursts, Radio Emission, Radio Spectra, Ultraviolet Radiation

Scientific paper

The detection and subsequent observations of the strongest radio source
associated with an RS CVn binary system, RT Lac, are reported. Like the
other detected RS CVn systems, its radio-emission mechanism is probably
nonthermal gyrosynchrotron radiation, though its radio spectrum may be
affected by thermal gas in the neighborhood of the system.

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