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AG Dra a Symbiotic Star With an Uncommon Cool Component

Published online by Cambridge University Press:  12 April 2016

M. Friedjung*
Affiliation:
Institut d’Astrophysique 98 bis, Bd Arago F-75014, PARIS

Summary

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AG Dra is probably a metal poor symbiotic binary of the galactic halo. The luminosity of the cool component is uncertain, which contributes to doubts about the correct model. Behaviour in activity is non classical with high ionization emission lines still having been seen then in the spectrum. This may perhaps most easily be explained by a weak thermonuclear event.

Type
Session 3. Physics of Individual Objects
Copyright
Copyright © Kluwer 1988

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