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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2577
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dc.contributor.authorMallik, D. C. V-
dc.date.accessioned2008-07-02T11:13:52Z-
dc.date.available2008-07-02T11:13:52Z-
dc.date.issued1991-
dc.identifier.citationProceedings Astronomical Society of Australia ,Vol. 9, No. 1, pp. 15 - 19en
dc.identifier.issn0066-9997-
dc.identifier.urihttp://hdl.handle.net/2248/2577-
dc.description.abstractThe review describes some of the progress made in observations and their interpretation, particularly in the context of the evolution of the nebulae and the central stars. It includes a discussion on the improved determinations of magnitudes and temperatures of the central stars, and of progress in the measurement of distances, and a reassessment of the observed mass-distribution of the central stars. The last topic is responsible for a large number of studies of central star evolutionen
dc.format.extent805603 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Australiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1991PASAu...9...15Men
dc.subjectAsymptotic giant branch starsen
dc.subjectPlanetary Nebulaeen
dc.subjectStellar Evolutionen
dc.subjectStellar Evolutionen
dc.subjectStellar Compositionen
dc.subjectStellar Magnitudeen
dc.subjectStellar Massen
dc.titlePlanetary nebulae - Origin and evolutionen
dc.typeArticleen
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