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Rapid evolution and nebula formation

Published online by Cambridge University Press:  25 May 2016

Garrelt Mellema
Garrelt Mellema*
Affiliation:
Stockholm Observatory

Extract

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The formation of a Planetary Nebula is determined by the star which lives and evolves in the middle of it. The star produces both the winds and the photons which determine the shape and appearance of the nebula. Here I study how the shape of the PN depends on the stellar properties.

Type
IV. Envelopes
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 263
Copyright
Copyright © Kluwer 1997 

References

Blöcker, T., 1995, A&A 299, 755.Google Scholar
Corradi, R.L.M., Schwarz, H.E. 1995, A&A 293, 871.Google Scholar
Mellema, G., 1995, MNRAS 277, 173.Google Scholar