Wind mass transfer in S-type symbiotic binaries - III. Confirmation of a wind focusing in EG Andromedae from the nebular [O III] λ5007 line

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Fig. 3.

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Example of observed Hα line profile, its fit by Eq. (2), and its individual components (Sect. 3.2) at different orbital phases. Vertical dotted line corresponds to the wavelength of the systemic velocity.

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