Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-26T03:52:53.605Z Has data issue: false hasContentIssue false

V367 Cyg as the interacting binary

Published online by Cambridge University Press:  12 April 2016

H. Schneider
Affiliation:
Universitäts-Sternwarte, Göttingen, F.R.G.
K. Pavlovski
Affiliation:
Hvar Observatory, Zagreb, Yugoslavia
M.C. Akan
Affiliation:
Ege University Observatory, Izmir, Turkey

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The interacting binary V367 Cyg is contained in the original list of W Serpentis stars discovered by Plavec and Koch (1978) in their initial UV study and has been subject of numerous studies, both photometric and spectroscopic.

Type
Research Article
Copyright
Copyright © Kluwer 1989

References

References:

Plaves, W.,Koch, R.H., 1978: IBVS No.1482 Google Scholar