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Ring Nebulae Around Massive Stars

Published online by Cambridge University Press:  03 August 2017

You-Hua Chu
You-Hua Chu*
Affiliation:
Astronomy Department, University of Illinois 1002 W. Green Street, Urbana, Illinois 61801 U. S. A.

Abstract

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Ring nebulae have been found around WR stars, OB and Of stars, and luminous blue variables. Ring nebulae are formed by the interaction between the central stars and their ambient medium via different combinations of stellar winds, ejecta, and radiation. The spectral properties of the nebulae can be used to diagnose the stellar properties, such as luminosity and effective temperature. Correlations between ring nebulae and their central stars may be used to check scenarios of stellar evolution.

Type
Session VI. Enrichment
Information
Symposium - International Astronomical Union , Volume 143: Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies , 1991 , pp. 349 - 364
Copyright
Copyright © Kluwer 1991 

References

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