Planetary nebulae with close binary central stars

Details Planetary nebulae with close binary central stars Planetary nebulae with close binary central stars

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...105...37l&link_type=abstract

Astronomy and Astrophysics, vol. 105, no. 1, Jan. 1982, p. 37-41.

Astronomy and Astrophysics

Astrophysics

56

Binary Stars, Planetary Nebulae, Stellar Evolution, Stellar Structure, Astronomical Models, Stellar Envelopes, Variable Stars

Scientific paper

The observational record concerning planetary nebulae with close binary nuclei is surveyed, in light of a model for the formation of such nebulae which predicts a characteristic, nonspherical morphology. Although agreement is found between the morphological prediction of the model and the observed shapes of M2-9, NGC 6164-5, and MZ 3, cases are found in which different observations yield different results with respect to central star variability.

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