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

Astronomy and Astrophysics – Astrophysics

Scientific paper

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To be published in the Proceedings of IAU Colloquium 169 on Variable and Non-Spherical Stellar Winds in Luminous Hot Stars, ed

Scientific paper

10.1007/BFb0106406

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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