Comments on the Formation of Elliptical Planetary Nebulae

Details Comments on the Formation of Elliptical Planetary Nebulae Comments on the Formation of Elliptical Planetary Nebulae

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...469..734s&link_type=abstract

Astrophysical Journal v.469, p.734

Astronomy and Astrophysics

Astronomy

10

Stars: Binaries: Close, Ism: Structure, Ism: Planetary Nebulae: General, Stars: Agb And Post-Agb

Scientific paper

We point to several problems in the recently proposed rotating extended envelope scenario for the formation of elliptical planetary nebulae. The problems that we find here add to the accumulated supporting evidence for the necessity to include the influence of companions in models for the formation of elliptical planetary nebulae. The binary companions need not necessarily be stars: they may be brown dwarfs or massive planets as well.

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