Asymmetrical Planetary Nebulae and Central Star Masses

Details Asymmetrical Planetary Nebulae and Central Star Masses Asymmetrical Planetary Nebulae and Central Star Masses

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.225..275a&link_type=abstract

Astrophysics and Space Science, Volume 225, Issue 2, pp.275-287

Astronomy and Astrophysics

Astrophysics

6

Scientific paper

PN morphology does not depend on the PN evolution stage. A much more
important dependence on PN mass class exists. Possibly, when the mass of
the parent star increases, then also increases the probability that the
star has an invisible low mass companion (brown dwarf or massive planet)
which determines the axisymmetrical morphology of the mass loss.

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