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On the Spectrum of VV Puppis

Published online by Cambridge University Press:  25 April 2016

D. T. Wickramasinghe  and
N. Visvanathan
D. T. Wickramasinghe
Affiliation:
Department of Applied Mathematics ANU
N. Visvanathan
Affiliation:
Mt. Stromlo and Siding Spring Observatories ANU
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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
Publications of the Astronomical Society of Australia , Volume 3 , Issue 5 , 1979 , pp. 311 - 312
Copyright
Copyright © Astronomical Society of Australia 1979

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References

Fabian, A.C., Pringle, J.E., and Rees, M.J., Mon. Not. R. Astron. Soc, 175, 43 (1976)Google Scholar
Liebert, J., and Stockman, H.S., (Preprint) (1979).Google Scholar
Liebert, J., Stockman, H.S., Angel, J.R.P., Woolf, N.J., Hege, K., and Margon, B., Astrophys. J., 225, 201 (1978).Google Scholar
Tapia, S., IAU Cire. No. 3054.Google Scholar
Trubinikov, B.A., Soviet Phys — Doklady, 3, 136 (1958).Google Scholar
Visvanathan, N., and Wickramasinghe, D.T., Nature, (submitted) (1979)Google Scholar
Wickramasinghe, D.T., and Visvanathan, N., Mon. Not. R. Astron. Soc. (submitted) (1979).Google Scholar