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A New Type of Asymmetric Outflow in the Recurrent Nova RS Oph in Quiescence
Published online by Cambridge University Press: 12 April 2016
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 km 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.
- Type
- Novae & Symbiotic Stars
- Information
- International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 331 - 332
- Copyright
- Copyright © Kluwer 1996