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Are Molecules Responsible for Origin of Cold Giants Mass Loss?

Published online by Cambridge University Press:  07 August 2017

I. K. Shmeld
Affiliation:
Radioastrophysical observatory Latvian Academy of Sciences Turgeneva 19, 226524 Riga, Latvia
V. S. Strelnitskij
Affiliation:
Institut for Astronomy Ac. Sci. USSR, Pjatnickaja 48, 109017 Moscow USSR
A. V. Fedorova
Affiliation:
Institut for Astronomy Ac. Sci. USSR, Pjatnickaja 48, 109017 Moscow USSR
O. V. Fedorova
Affiliation:
Institut for Astronomy Ac. Sci. USSR, Pjatnickaja 48, 109017 Moscow USSR

Abstract

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It is shown that radiative pressure in vibronic transitions of molecules may play an important role in origin of mass outflow of cold giants and supergiants.

Type
Near Stellar Environments
Copyright
Copyright © Kluwer 1992 

References

REFERENCES

Dominik, C. et. al., (1990) Astron. and Astroph., 240., 365.Google Scholar
Hearn, A. G. (1989) in: “From Miras to Planetary Nebulae: which Path for Stellar Evolution” - Proc. of International Colloqium. Sept. 4-7. Montpellier France.Google Scholar
Tsuji, T. (1966) Publ. Astron. Soc. Jap., 18, N3, 127.Google Scholar