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59 Cygni: A Tilted ϕ Persei like System
Published online by Cambridge University Press: 12 April 2016
Abstract
The binarity of 59 Cygni was confirmed and orbital parameters from the radial velocity curve of the primary derived. The observed emission variability resembles the one of ɸ Per in quite some detail, suggesting a similar nature of the companion: a hot, compact star.
- Type
- 6. Disks
- Information
- International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 581 - 584
- Copyright
- Copyright © Astronomical Society of the Pacific 2000
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