Abstract
In the spectral range λλ5800–8750, HBV 475 shows important spectral variations between 1969 and 1974. Sometimes the “hot component” spectrum dominates (many emission lines), sometimes the “cool component” is preponderent (many molecular absorption TiO bands) (Andrillat 1973 — Andrillat, Houziaux 1976).
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Andrillat, Y.: 1973, Mém.Soc.Roy.Sci.Liège, T.5, 371.
Andrillat, Y., Houziaux, L.: 1976, Astron.Astrophys. 5, 119.
Andrillat, Y., Vreux, J.M., Dennefeld, M.: 1982, IAU Symp. 99 (forthcoming).
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© 1982 D. Reidel Publishing Company, Dordrecht, Holland
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Andrillat, Y. (1982). Variability of HBV 475 in the near Infrared. In: Friedjung, M., Viotti, R. (eds) The Nature of Symbiotic Stars. Astrophysics and Space Science Library, vol 95. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7834-8_29
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DOI: https://doi.org/10.1007/978-94-009-7834-8_29
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