Spectrophotometry of RS Canum Venaticorum, AR Lacertae, and UX ARIETIS

Details Spectrophotometry of RS Canum Venaticorum, AR Lacertae, and UX ARIETIS Spectrophotometry of RS Canum Venaticorum, AR Lacertae, and UX ARIETIS

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...216..503r&link_type=abstract

Astrophysical Journal, Part 1, vol. 216, Sept. 1, 1977, p. 503-507.

Astronomy and Astrophysics

Astrophysics

17

Eclipsing Binary Stars, Stellar Envelopes, Stellar Spectrophotometry, Ultraviolet Spectroscopy, Emission Spectra, High Temperature Gases, Hydrogen, Wavelengths

Scientific paper

The wavelength dependences of the ultraviolet excesses of the RS CVn-type stars RS CVn, AR Lac, and UX Ari have been measured spectrophotometrically with a wavelength resolution of 60 A. A number of mechanisms are examined to account for the excess light from these systems, and it is concluded that free-free emission from hot circumstellar gas provides the most satisfactory explanation.

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