No CrossRef data available.
Article contents
The peculiar symbiotic object V1329 Cygni: single-star versus binary models
Published online by Cambridge University Press: 12 April 2016
Extract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
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
Grygar, J., Hric, L., Chochol, D., Mammano, A.: 1979, Bull. astr. Inst. Czechosl. 30, 308
Google Scholar