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From What Radius Do the Winds of Magellanic Cloud Supergiants Produce Fe II Emission Lines?

Published online by Cambridge University Press:  04 August 2017

M. Friedjung  and
C. Muratorio
M. Friedjung
Affiliation:
Institut d'Astrophysique, Paris, France and Observatoire de Marseille, Marseille, France
C. Muratorio
Affiliation:
Institut d'Astrophysique, Paris, France and Observatoire de Marseille, Marseille, France

Abstract

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Maximum values for the inner radii at which Fe II emission line formation can take place in the winds of three Magellanic Cloud supergiants have been determined. The lie between 3 × 1013 and 3 × 1014 for R50, R82, and R126.

Type
Stellar Populations
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 235 - 236
Copyright
Copyright © Reidel 1984 

References

Friedjung, M., Muratorio, A. 1980, Astron. Astrophys, 85 233 Google Scholar
Viotti, R. 1976, Astrophys. J. 204 293 Google Scholar