CN 1-1 - A bipolar type I planetary nebula

Details CN 1-1 - A bipolar type I planetary nebula CN 1-1 - A bipolar type I planetary nebula

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...214..331b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 214, no. 1-2, April 1989, p. 331, 332.

Astronomy and Astrophysics

Astronomy

3

Planetary Nebulae, Polarization Characteristics, Abundance, Cosmic Dust, Infrared Astronomy Satellite, Symbiotic Stars

Scientific paper

Polarization measurements of Cn 1-1 are interpreted as due to scattering
by nebular dust. It is suggested that the nebula has a bipolar
morphology. This, together with the enhanced nitrogen abundance in the
nebula, supports the view that Cn 1-1 is a type I protoplanetary nebula.

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