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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3007
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dc.contributor.authorMallik, D. C. V-
dc.date.accessioned2008-08-05T07:22:16Z-
dc.date.available2008-08-05T07:22:16Z-
dc.date.issued1983-
dc.identifier.citationD. R. Flower. ed., Planetary nebulae, Proceedings of the 103 Symposium of the International Astronomical Union, Held at University college, London, U. K. August 9 – 13, 1982en
dc.identifier.urihttp://hdl.handle.net/2248/3007-
dc.description.abstractThe electron density, temperature and ion abundances in the nebulae surrounding the two WC 10 stars CPD-56 deg 8032 and He2-113 have been estimated. In CPD-56 deg 8032 sulphur, nitrogen and oxygen seem to have solar abundances, whereas carbon and neon are enhanced. The nebular properties of all the four WC 10 stars He2-113, CPD-56 deg 8032, M4-18 and V348 Sgr are compared.en
dc.format.extent260241 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherInternational Astronomical Unionen
dc.relation.ispartofseriesInternational Astronomical Union Symposium No. 103-
dc.relation.urihttp://adsabs.harvard.edu/abs/1983IAUS..103..424Men
dc.subjectPlanetary Nebulaeen
dc.subjectIon density (concentration)en
dc.subjectPlanetary nebulaeen
dc.titleBirthrate of Planetary Nebulaeen
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