Fig. 3.
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Sample Hα profiles of RS Oph (from data in Munari & Valisa 2022) early in the outburst and at the time of our EVN radio imaging (see Sect. 3.3 for details). Heliocentric radial velocities are given at the top of the panels. The arrow in the top panel marks the −4700 km s−1 terminal velocity of the P-Cyg absorption, while the orange line in the lower panel is a fit to the broad pedestal extending up to −4200 km s−1.
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