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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

A. Bianchini ,
M. Friedjung  and
F. Sabbadin
A. Bianchini
Affiliation:
Osservatorio Astronomico, 35100-Padova, Italy
M. Friedjung
Affiliation:
Institut d’Astrophysique, 98bis, Bd Arago, 75014 Paris, France
F. Sabbadin
Affiliation:
Osservatorio Astronomico, 35100-Padova, Italy

Abstract

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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

References

- Bianchini, A.,Friedjung, M. and Sabbadin, F., 1985a.Inf.Bull.Var.Stars N.2650.Google Scholar
- Bianchini, A.,Friedjung, M. and Sabbadin, F., 1985b. In:Recent Results on Cataclysmic Variables, p.77, ESA SP-236.Google Scholar
- Duerbeck, H.W.,Scitter, W.S.and Duemmler, R., 1987. Mon. Not. R. astr. Soc. 229, 653.Google Scholar
- Warner, B., 1985.Mon. Not. R. astron. Soc. 217, 1P Google Scholar