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The Symbiotic Novae

Published online by Cambridge University Press:  12 April 2016

Roberto Viotti*
Affiliation:
Istituto Astrofisica Spaziale, CNR, Frascati

Abstract

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A small number of symbiotic stars are characterized by a single nova-like outburst with a very slow time evolution and several years of permanence at maximum. We describe in detail RR Tel and discuss the main properties of these objects.

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

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