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Bolometric Light Curves of Symbiotic Novae

Published online by Cambridge University Press:  07 August 2017

U. Mürset  and
H. Nussbaumer
U. Mürset
Affiliation:
Institute of Astronomy ETH-Zentrum CH-8092 Zürich Switzerland
H. Nussbaumer
Affiliation:
Institute of Astronomy ETH-Zentrum CH-8092 Zürich Switzerland

Abstract

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We determine bolometric light curves and total energies radiated away during the outburst of symbiotic novae. Time integrated lower limits to the total energy of 0.9×1046 <E[erg] < 7×1046 are found. Thus, the output is comparable to, or larger than the total energy production of a classical nova outburst. From the mass-luminosity relation we find the underlying stellar masses to be 0.5 < M/M ⊙ < 1.1.

Type
Oral and Contributed Papers
Information
Symposium - International Astronomical Union , Volume 151: Evolutionary Processes in Interacting Binary Stars , 1992 , pp. 435 - 438
Copyright
Copyright © Kluwer 1992 

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