Abstract
AbstractThe 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.
Publisher
Cambridge University Press (CUP)
Reference8 articles.
1. Transient emission events in the early Be star 59 Cygni
2. Štefl S. , Hummel W. , Rivinius Th. 1999, A&A submitted
Cited by
2 articles.
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