Velocity curves for broad and sharp components observed in the emission lines from AM Herculis

Astronomy and Astrophysics – Astrophysics

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Astronomical Spectroscopy, Binary Stars, Emission Spectra, Spectral Resolution, Stellar Spectra, X Ray Sources, Helium, Helium Atoms, Photon Density, Velocity Distribution

Scientific paper

High-resolution observations of the profiles of the He I 4471-A and He II 4686-A emission lines have been obtained around a complete cycle of the X-ray binary AM Her. The profiles are resolved into broad (B) and sharp (S) components; velocity curves are given for each component for both the He I and He II lines. The velocity amplitude of the B component is about 4 times that of the S component. The two components vary out of phase by 133 (+ or -5) deg. The S component is at conjunction during the soft X-ray eclipse. Implications of these results for models of AM Her are discussed.

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