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Time-Resolved Optical Spectroscopy of V795 Herculis
Published online by Cambridge University Press: 12 April 2016
Abstract
High resolution optical spectroscopy of V795 Herculis shows complex time- and phase-dependent behaviour of the disk emission. Separate low- and high-velocity fluctuations phased on the 2.6 hr orbital period are observed in the wings of the Balmer lines, prompting a gas stream overflow model.
- Type
- Part 15. Poster Papers
- Information
- International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 697 - 698
- Copyright
- Copyright © Astronomical Society of the Pacific 1997