Hostname: page-component-78c5997874-94fs2 Total loading time: 0 Render date: 2024-11-06T09:13:24.039Z Has data issue: false hasContentIssue false
  • English
  • Français

Are Molecules Responsible for Origin of Cold Giants Mass Loss?

Published online by Cambridge University Press:  07 August 2017

I. K. Shmeld ,
V. S. Strelnitskij ,
A. V. Fedorova  and
O. V. Fedorova
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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Information
Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 413 - 414
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