Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3658
Title: CN 1-1 - A bipolar type I planetary nebula
Authors: Bhatt, H. C
Keywords: Planetary Nebulae;Polarization Characteristics;Abundance;Cosmic Dust;Infrared Astronomy Satellite;Symbiotic Stars
Issue Date: Apr-1989
Publisher: European Southern Observatory
Citation: Astronomy and Astrophysics, Vol. 214, No. 1 - 2, pp. 331 - 332
Abstract: 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.
URI: http://hdl.handle.net/2248/3658
ISSN: 0004-6361
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Appears in Collections:IIAP Publications

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