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“Two New States” of VV Puppis

Published online by Cambridge University Press:  12 April 2016

N. Visvanathan  and
D. T. Wickramasinghe
N. Visvanathan
Affiliation:
Mount Stromlo and Siding Spring Observatories, Research School of Physical Sciences, The Australian National University
D. T. Wickramasinghe
Affiliation:
Applied Mathematics Department, The Australian National University

Extract

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VV Puppis, a dwarf-nova binary with a 100 min period (Herbig 1960) was observed on two occasions. On 2nd February 1979, VV Puppis was in a faint inactive state. On the other hand it was bright and active on 14th June 1979. Spectral and polarimetry observations were made on both these occasions using IDS (modified as polarimeter) at the f/15 Cassegrain focus of the 4 meter Anglo-Australian Telescope. Spectral range covered was from 3600 Å to 7000 Å with a resolution of 10 Å. The star and sky apertures both were of size 3 × 4 sec of arc and 40 sec apart.

Type
Colloquium Session V
Information
International Astronomical Union Colloquium , Volume 53: White Dwarfs and Variable Degenerate Stars , August 1979 , pp. 330 - 333
Copyright
Copyright © The University of Rochester 1979

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