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- W4299847593 abstract "We present the first results of a continuous monitoring of Algol with IUE along 1.5 orbital period (4 1/3 days). A total of 32 high resolution spectra were obtained. Algol represents the final slow stage of mass transfer. The spectra show the presence of high ionization lines (NV, SiIV, CIV) due to the heating of the gas that impacts the accreting star. The depth of the primary eclipse is larger at shorter wavelengths and the shape of the continuum out of the eclipse is compatible with a B star, ruling out the presence of an extra light source at these wavelengths." @default.
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- W4299847593 date "1992-01-01" @default.
- W4299847593 modified "2023-10-17" @default.
- W4299847593 title "First Results of Continuous IUE Observations of Algol" @default.
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- W4299847593 doi "https://doi.org/10.1017/s0074180900122302" @default.
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