Abstract
H I emission lines in the spectrum of the recurrent nova and symbiotic star RS Oph in quiescence are sometimes accompanied by blue-or red-shifted broad emission components. The displacements of the broad components from the narrow lines change from -1300 to +1200 s-1, but possibly not continuously. The broad components seem to appear in some restricted regions on the spectra. An asymmetry between the blue-and red-shifts is noticed.
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