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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/332
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dc.contributor.authorMallik, D. C. V-
dc.date.accessioned2005-02-09T02:01:56Z-
dc.date.available2005-02-09T02:01:56Z-
dc.date.issued1982-06-
dc.identifier.citationBASI, Vol. 10, No. 2, pp. 73-110en
dc.identifier.urihttp://hdl.handle.net/2248/332-
dc.descriptionOpen Access-
dc.description.abstractRecent research on planetary nebulae is reviewed, with special emphasis on ultraviolet and infrared observations. Various distance scales and statistics based on them are discussed and the emperical mass-radius relation due to Maciel & Pottasch (1980) is used to compile a new list of local planetaries. Recent determinations of the effective temperatures of central stars and their new locations onthe H-R diagram are described. The implications of the chemical abundance studies of these nebulae are discussed in the light of current work on stellar evolution and nucleosynthesis.en
dc.format.extent4093217 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectPlanetary Nebulae Statisticsen
dc.subjectAbundancesen
dc.subjectStellar Evolutionen
dc.titlePlanetary nebulaeen
dc.typeArticleen
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