The Peculiar Symbiotic Object V1329 Cygni: Single-Star Versus Binary Models

  • Jiri Grygar
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 95)


The variable emission-line object V1329 Cyg (= HBV 475) was discoverred 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.


Emission Line Stellar Wind Symbiotic Star Binary Hypothesis Radial Velocity Data 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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Copyright information

© D. Reidel Publishing Company, Dordrecht, Holland 1982

Authors and Affiliations

  • Jiri Grygar
    • 1
    • 2
  1. 1.Astronomical InstituteSlovak Academy of SciencesTatranska LomnicaCzechoslovakia
  2. 2.Institute of PhysicsCzechoslovak Academy of SciencesRez Drahomir ChocholCzechoslovakia

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