Ultraviolet to near-infrared continuum flux distribution in the active binary RS Canum Venaticorum

Details Ultraviolet to near-infrared continuum flux distribution in the active binary RS Canum Venaticorum Ultraviolet to near-infrared continuum flux distribution in the active binary RS Canum Venaticorum

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.169..233g&link_type=abstract

(IAU, European Regional Astronomy Meeting on New Windows to the Universe, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics a

Astronomy and Astrophysics

Astrophysics

2

Eclipsing Binary Stars, Near Infrared Radiation, Ultraviolet Radiation, Astronomical Catalogs, Iue, Stellar Luminosity, Stellar Spectrophotometry

Scientific paper

We present multifrequency observations of the active binary RS CYn. Ultraviolet observations were obtained from the IUE data bank. Optical observations were made at the Observatorio del Roque de los Muchachos (La Palma), while the infrared observations were obtained at the Observatorio del Teide (Tenerife). The continuum of RS CVn shows that both components behave in good agreement with normal values for their spectral type and luminosity class, when observed data are corrected for small spot effects. No significant circumstellar reddening is detected

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