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The peculiar symbiotic object V1329 Cygni: single-star versus binary models

Published online by Cambridge University Press:  12 April 2016

Jiri Grygar  and
Drahomir Chochol
Jiri Grygar
Affiliation:
Institute of Physics, Czechoslovak Academy of Sciences, Rez Drahomir Chochol
Drahomir Chochol
Affiliation:
Astronomical Institute, Slovak Academy of Sciences, Tatranska Lomnica, Czechoslovakia

Extract

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The variable emission-line object V1329 Cyg (= HBV 475) was discover red by Kohoutek (1969).Crampton and Grygar (1969) identified more than 100 emission lines in the blue portion of the spectrum, while Andrillat (1969) found evidence for the late-type (M) spectrum in the near infrared. This justified the classification of the object among the symbiotic stars. The classification was subsequently confirmed by all authors who studied the spectroscopic evolution of the object.

Type
Session II – Discussion on Individual Stars
Information
International Astronomical Union Colloquium , Volume 70: The Nature of Symbiotic Stars , 1982 , pp. 165 - 168
Copyright
Copyright © Reidel 1982

References

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