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Time Resolved Optical Spectroscopy of V795 Her
Published online by Cambridge University Press: 12 April 2016
Abstract
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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.
- Type
- Non-Magnetic Cataclysmic Variables
- Information
- International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 41 - 42
- Copyright
- Copyright © Kluwer 1996
References
Haswell, C.A., Horne, K., Thomas, G., et al. 1994, in “Interacting Binary Stars”, ed. Shatter, A., ASP Conf. Ser.
56, 268
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