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Spectroscopic Observations of the Southern Old Novae CP Pup and V841 Oph
Published online by Cambridge University Press: 12 April 2016
Abstract
New spectroscopic observations of the old nova CP Pup suggest most probable orbital period of 0.061375 days. First systematic monitoring of the very old nova V841 Oph reveals orbital motion with a most probable period of about 0.6 days. A slightly eccentric solution at P = 0.3755 days is less probable.
- Type
- 1a. Basic Properties of Novae
- Information
- International Astronomical Union Colloquium , Volume 122: Physics of Classical Novae , 1990 , pp. 61 - 62
- Copyright
- Copyright © Springer-Verlag 1990
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