0124699 - ASU-R 20000158 RIV US eng C - Konferenční příspěvek (zahraniční konf.)
Rivinius, T. - Štefl, Stanislav
59 Cygni: A tilted .phi. Persei like System.
The Be phenomenon in early-type stars. San Francisco: Astronomical Society of the Pacific, 2000 - (Smith, M.; Henrichs, H.; Fabregat, J.), s. 581-584
[Colloquium of the International Astronomical Union /175./. Alicante (ES), 28.06.1999-02.07.1999]
Výzkumný záměr: CEZ:AV0Z1003909
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika

The binary of 59 Cygni was confirmed and orbital parametrs from the radial velocity curve of the primary derived. The observed emission variability resembles the one .phi. Per in quite some details, suggesting a similar nature of the companion: a hot, compact star.
Trvalý link: http://hdl.handle.net/11104/0022958