1. IIA Institutional Repository
  2. IIAP Publications
  3. IIAP Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3658
Full metadata record
DC FieldValueLanguage
dc.contributor.authorBhatt, H. C-
dc.date.accessioned2008-09-16T14:37:16Z-
dc.date.available2008-09-16T14:37:16Z-
dc.date.issued1989-04-
dc.identifier.citationAstronomy and Astrophysics, Vol. 214, No. 1 - 2, pp. 331 - 332en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/3658-
dc.description.abstractPolarization 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.en
dc.language.isoenen
dc.publisherEuropean Southern Observatoryen
dc.relation.urihttp://ads.iucaa.ernet.in/abs/1989A%26A...214..331Ben
dc.subjectPlanetary Nebulaeen
dc.subjectPolarization Characteristicsen
dc.subjectAbundanceen
dc.subjectCosmic Dusten
dc.subjectInfrared Astronomy Satelliteen
dc.subjectSymbiotic Starsen
dc.titleCN 1-1 - A bipolar type I planetary nebulaen
dc.typeArticleen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
CN 1-1 - A bipolar type I planetary nebula344.03 kBAdobe PDFView/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.