A study of CQ Cephei: Far UV to infrared

Details A study of CQ Cephei: Far UV to infrared A study of CQ Cephei: Far UV to infrared

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.176..335s&link_type=abstract

In ESA 3rd European IUE Conf. p 335-338 (SEE N83-11889 02-88)

Computer Science

1

Binary Stars, Cepheid Variables, Far Ultraviolet Radiation, Infrared Spectra, Stellar Spectra, Iue, Light Curve, Stellar Spectrophotometry, Stellar Structure, Stellar Winds, Ultraviolet Spectra, Wolf-Rayet Stars

Scientific paper

Reappraisal of old optical spectrograms and photometry of the close binary Wolf-Rayet (WR) star, CQ Cephei, was combined with optical and infrared photometry and high and low resolution data from IUE. Data suggest that the companion to the WN7 star is at least partially immersed in the WR wind. However, the nature of the companion is not positively established.

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