Modulation of short-period oscillations and colour asymmetry in pulsed emission lines - A structural interpretation of recent observations of DQ HER

Astronomy and Astrophysics – Astronomy

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Eclipsing Binary Stars, Emission Spectra, Line Spectra, Oscillations, Pulsed Radiation, Stellar Spectra, Asymmetry, Color, Helium, Novae, Stellar Luminosity, Stellar Mass Accretion, Stellar Rotation, Ultraviolet Radiation, White Dwarf Stars

Scientific paper

The dependence of the amplitude and phase of the 71-s oscillations in DQ Her on the system's binary phase, observed by Patterson, Robinson, and Nather (1978), are interpreted in terms of obscuration by structure on the edge of the accretion disk. It is argued that such obscuration, in conjunction with the eclipses, will lead to the asymmetry in the He II 4686-A emission-line profile reported by Chanan, Nelson, and Margon (1978).

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