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Time Resolved Optical Spectroscopy of V795 Her

  • R. J. Dickinson (a1), R. K. Prinja (a1), S. R. Rosen (a2) and K. Horne (a3)

Abstract

We present high resolution optical spectroscopy of the cataclysmic variable (CV) V795 Her. The time- and phase- dependent behaviour of the emission source is examined using two-dimensional image analysis and Doppler reconstruction techniques on the orbital profiles. A clear S-wave modulation of a weak emission feature in the Hβ and Hγ line wings (extending to ~1800 km s−1) is present, with complex asymmetric properties.

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Copyright

References

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Haswell, C.A., Horne, K., Thomas, G., et al. 1994, in “Interacting Binary Stars”, ed. Shatter, A., ASP Conf. Ser. 56, 268
Prinja, R.K., Drew, J.E., Rosen, S.R., 1992, MNRAS, 256, 219
Rosen, S., Prinja, R.K., Drew, J.E., 1996, these proceedings, p43

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