Article contents
On the Spectrum of VV Puppis
Published online by Cambridge University Press: 25 April 2016
Extract
Since the discovery of variable circular and linear polarisation in VV Puppis (Tapia 1977), several investigators have observed the system. The new observations particularly of polarisation (Liebert et al. 1978, Liebert and Stockman 1979 have ruled out the standard dwarf nova (accretion disc — hot spot) model previously used to interpret the light curve of VV Puppis.
- Type
- Contributions
- Information
- Copyright
- Copyright © Astronomical Society of Australia 1979
References
- 2
- Cited by