On the origin of planetary nebulae

Details On the origin of planetary nebulae On the origin of planetary nebulae

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...110l...1n&link_type=abstract

Astronomy and Astrophysics, vol. 110, no. 1, June 1982, p. L1, L2.

Astronomy and Astrophysics

Astrophysics

4

Magnetic Flux, Planetary Nebulae, Stellar Evolution, Stellar Magnetic Fields, Stellar Mass Ejection, Stellar Winds, Red Giant Stars, White Dwarf Stars

Scientific paper

It is suggested that randomly emerging magnetic flux may be responsible for the ejection of the planetary nebula and for the stellar wind emanating from the central stars of such nebulas. The theoretical basis of this mechanism is briefly analyzed, and symbiotic stars and Mira type red giants, as well as NGC 6543, are cited as examples supporting the notion that magnetic fields strong enough to cause the mass loss involved in the formation of a planetary nebula exist.

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