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59 Cygni: A Tilted ϕ Persei like System

Published online by Cambridge University Press:  12 April 2016

Th. Rivinius  and
S. Štefl
Th. Rivinius
Affiliation:
Landessternwarte Königstuhl, D-69117 Heidelberg, Germany
S. Štefl
Affiliation:
Astronomical Institute, Academy of Sciences, CZ-251 65 Ondřejov, Czech Republic

Abstract

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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

References

Barker, P.K. 1983, AJ 88, 72;Google Scholar
Doazan, V., Grady, C.A., Snow, T.P., et al. 1985, A&A 152, 182 Google Scholar
Doazan, V., Barylak, M., Rusconi, L., et al. 1989, A&A 210, 249 Google Scholar
Gies, D.R., Willis, C.Y., Penny, L.R., et al. 1993, PASP 105, 281 Google Scholar
Hummel, W. 1998, A&A 330, 243 Google Scholar
Kaufer, A. 1998, In: Reviews in Modem Astronomy 11, ed. Schielicke, R., p. 177 Google Scholar
Štefl, S., Hummel, W., Rivinius, Th. 1999, A&A submittedGoogle Scholar
Tarasov, A.E., Tuominen, I. 1987, Proc. Reg. Eur. IAU Meet., Publ. Astron. Inst. Czechosl. Acad. Sc. 5, 70, p.127, ed.: Harmanec, P. Google Scholar