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Slingshot Prominences During Dwarf Nova Outbursts?

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Cataclysmic Variables and Related Objects

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 208))

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Abstract

We present phase-resolved spectroscopy of two dwarf novae, IP Peg and SS Cyg, observed in outburst with the WHT/ISIS spectropolarimeter. Doppler tomograms of several emission lines show peculiar narrow, stationary emission components.

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References

  • Horne, K., 1991, in “Fundamental Properties of CVs” ed. A.W. Shatter (U. San Diego)

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Author information

Authors and Affiliations

  1. Astronomical Institute, Utrecht University, The Netherlands

    D. Steeghs

  2. Physics & Astronomy, University of St.Andrews, UK

    K. Horne

  3. Astronomy Group, University of Southampton, UK

    T. R. Marsh

Authors
  1. D. Steeghs
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  2. K. Horne
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  3. T. R. Marsh
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Editor information

Editors and Affiliations

  1. Keele University, UK

    A. Evans  & Janet H. Wood  & 

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© 1996 Kluwer Academic Publishers

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Steeghs, D., Horne, K., Marsh, T.R. (1996). Slingshot Prominences During Dwarf Nova Outbursts?. In: Evans, A., Wood, J.H. (eds) Cataclysmic Variables and Related Objects. Astrophysics and Space Science Library, vol 208. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0325-8_20

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  • DOI: https://doi.org/10.1007/978-94-009-0325-8_20

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6632-7

  • Online ISBN: 978-94-009-0325-8

  • eBook Packages: Springer Book Archive

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