IUE observations of the 1982-84 eclipse of Epsilon Aurigae

Details IUE observations of the 1982-84 eclipse of Epsilon Aurigae IUE observations of the 1982-84 eclipse of Epsilon Aurigae

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985eepa.rept...37a&link_type=abstract

In NASA, Washington The 1982-1984 Eclipse of Epsilon Aurigae p 37-42 (SEE N86-12168 02-89)

Astronomy and Astrophysics

Astronomy

2

Auriga Constellation, Eclipsing Binary Stars, Iue, Light Curve, Spaceborne Astronomy, Spectral Energy Distribution, Broadband, High Dispersion Spectrographs, Occultation, Spectra, Ultraviolet Radiation, Wavelengths

Scientific paper

The major characteristics in the ultraviolet of the 1982-84 eclipse of Eps Aur as observed with IUE by various workers are summarized. This star can be observed over the entire IUE wavelength range, from 1200 to 3200 A, in low dispersion, allowing eclipse light curves to be obtained in broadband regions, but due to its steep spectral gradient and the sensitivities of IUE cameras, high resolution exposures adequately cover only the regions from 1700-1900 and 2400-3200 A. In many ways, the UV data confirms or expands upon interpretations of the stem made from observations in other wavelength regions, but in other respects the system remains as enigmatic as before.

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