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Mass loss from Eta Carinae

Published online by Cambridge University Press:  14 August 2015

C. D. Andriesse  and
R. Viotti
C. D. Andriesse
Affiliation:
Kapteyn Astronomical Institute, Roden, The Netherlands
R. Viotti
Affiliation:
Laboratorio di Astrofisica Spaziale, Frascati, Italy

Abstract

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This high luminosity (5 × 106 L⊙) star since 1840 is losing mass at the rate of 7.5 × 10−2 M⊙ per year. The large mass loss could be the result of vibrational instabilities produced in the CNO hydrogen burning phase of a very massive (160 M⊙) star. The presence of high excitation lines in the ultraviolet spectrum of Eta Car suggests the idea of a hot zone excited by dissipation of the supersonic turbulent flow.

Type
Session 1: Optical Spectroscopy
Information
Symposium - International Astronomical Union , Volume 83: Mass Loss and Evolution of O-Type Stars , 1979 , pp. 47 - 50
Copyright
Copyright © Reidel 1979 

References

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