"Wolf-Rayet and LBV Nebulae as the Result of Variable and Non-Spherical Stellar Winds"

Mordecai-Mark Mac Low
Max-Planck-Institut für Astronomie

To be published in the Proceedings of IAU Colloquium 169 on Variable and Non-Spherical Stellar Winds in Luminous Hot Stars, ed. B. Wolf (Springer-Verlag, Berlin, Heidelberg). Submitted 21 September 1998

The physical basis for interpreting observations of nebular morphology around massive stars in terms of the evolution of the central stars is reviewed, and examples are discussed, including NGC 6888, OMC-1, and eta Carinae.

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Last modified: Mon 21 Sept 1998