Computer Science
Scientific paper
Sep 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985eepa.rept...81a&link_type=abstract
In its The 1982-1984 Eclipse of Epsilon Aurigae p 81-90 (SEE N86-12168 02-89)
Computer Science
Auriga Constellation, Eclipsing Binary Stars, Iue, Light Scattering, Spectrum Analysis, Ultraviolet Spectra, Companion Stars, Dwarf Stars, Gratings (Spectra), Hot Stars, Wavelengths
Scientific paper
As a result of this work it was found that light scattered from the longer wavelengths constitutes a small but non-negligible, wavelength and time dependent fraction of the measured flux in the far UV. The reality of the UV excess has not been unambigiously ruled out. However, it is noted that there are still uncertainties in the assumed scattering profile. New measurements of the scattering properties of the cross disperser grating are planned in order to verify the results of Mount and Fastie and extend the wavelength coverage into the far wings of the profile. The results of these measurements will no doubt reduce some of these uncertainties. For the present, it is felt that the BCH approach is a significant improvement over the methods heretofore available for the treatment of scattered light in IUE spectra.
Aitner B.
Chapman Robert Dewitt
Kondo Yoshihiko
Stencel Robert E.
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