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IUE Observations of Z Andromedae

Published online by Cambridge University Press:  14 August 2015

M. Friedjung
M. Friedjung*
Affiliation:
Institut d'Astrophysique, Paris, France

Abstract

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The preliminary results of a joint study of this symbiotic star with 6 Italian astronomers are reported. The relative intensities of the intercombination emission lines indicate electron densities of 1010 and an upper limit to the dilution factor between 10−4 and 10−6. The resonance emission lines give a maximum thickness in the line of sight. A hot (T between 19000° and 26000°) continuum is interpreted as coming from a hot subdwarf, but the high excitation emission lines appear to be formed near the cool giant component of what is probably a close binary.

Type
X. … and The Rest (Symbiotics, Supergiants, Planetaries, Population II Systems)
Information
Symposium - International Astronomical Union , Volume 88: Close Binary Stars: Observations and Interpretation , 1980 , pp. 543 - 546
Copyright
Copyright © Reidel 1980 

References

Bohlin, R.C., Holm, A., Carnochan, D., Snijders, M.A.J., 1978, IUE Project Report.Google Scholar
Boyarchuk, A.A., 1967, Astr. Zh. 44, 1016.Google Scholar
Boyarchuk, A.A., 1969, in “Non Periodic Phenomena in variable Stars” Academic Press, Budapest, p. 395 Google Scholar
Boyarchuk, A.A., 1970, Iz Krim. Astrophys. Obs. 42, 264.Google Scholar
Flower, D.R., Nussbaumer, H., 1975, Astron. & Astrophys. 45, 145.Google Scholar
Linsky, J.L., Haisch, B.M., 1979, Astrophys. J., 229, L 27 CrossRefGoogle Scholar
Vernazza, J.E., Mason, E.H., 1978, Astrophys. J., 226, 720 Google Scholar
Yang, L.K., Nicholls, R.W., Morgan, F.J., 1975, Solar Phys., 45, 351.Google Scholar