Low Mass Stars Interacting with their Environment: the Formation of Planetary Nebulae

Details Low Mass Stars Interacting with their Environment: the Formation of Planetary Nebulae Low Mass Stars Interacting with their Environment: the Formation of Planetary Nebulae

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cokon.100..377m&link_type=abstract

Communications of the Konkoly Observatory, No. 100 (Vol. XII, 2), p. 377-386 (1997)

Physics

Scientific paper

This review gives a brief introduction to the subject of the formation of planetary nebulae. I describe the PN phase and the phases leading to it, concentrating on mass loss and circumstellar material. Next I describe the mechanism by which PNe are thought to form, the interacting stellar wind model. I end with a discussion of the origin of the aspherical shapes seen in the majority of PNe.

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