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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 

References

Austin, S., Starrfield, S., Saizar, P., Shore, S.N., Sonneborn, G.: 1990, in Evolution in Astrophysics , ESA SP-310, p. 367 Google Scholar
Lundmark, K.: 1921, Astronomische Nachrichten , 213, 94 Google Scholar
Mürset, U., Nussbaumer, H.: 1991, Astron. Astrophys. (in preparation) Google Scholar
Mürset, U., Nussbaumer, H., Schmid, H.M., Vogel, M.: 1991, Astron. Astrophys. (in press), (MNSV) Google Scholar
Nussbaumer, H.: 1991, in IAU Symposium No. 151, (this volume) CrossRefGoogle Scholar
Nussbaumer, H., Vogel, M.: 1990, Astron. Astrophys. 236, 117 Google Scholar
Nussbaumer, H., Vogel, M.: 1991, Astron. Astrophys. (in press) Google Scholar
Paczynski, B.: 1971, Acta Astr. 21, 417 Google Scholar
Payne-Gaposchkin, C., Gaposchkin, S.: 1938, Variable Stars , Harvard Obs. Monograph No. 5, p. 263 Google Scholar