Atmospheric eclipse effects in Wolf-Rayet binaries in the Small Magellanic Cloud

Details Atmospheric eclipse effects in Wolf-Rayet binaries in the Small Magellanic Cloud Atmospheric eclipse effects in Wolf-Rayet binaries in the Small Magellanic Cloud

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.281a.197k&link_type=abstract

In ESA, A Decade of UV Astronomy with the IUE Satellite, Volume 1 p 197-199 (SEE N89-10682 01-89)

Astronomy and Astrophysics

Astronomy

Eclipsing Binary Stars, Iue, Magellanic Clouds, Spaceborne Astronomy, Ultraviolet Astronomy, Ultraviolet Spectra, Metallicity, Stellar Atmospheres

Scientific paper

Results of IUE observations of three SMC W-R binary systems are presented. Selective atmospheric eclipse effects are evident in HD5980 (WN4+06I) and Sk 188 (W04+04V), and are very weak, or absent in Sk 108 (WN3+06I). The difference in heavy-metal content between the SMC and Galactic objects is clearly manifest in the lack of atmospheric eclipse effects in the wavelength range 1360 to 1470 A in HD5980 and Sk 188.

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