Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3784
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dc.contributor.authorAnandarao, B. G-
dc.contributor.authorBanerjee, D. P. K-
dc.contributor.authorDesai, J. N-
dc.contributor.authorJain, S. K-
dc.contributor.authorMallik, D. C. V-
dc.date.accessioned2008-09-22T16:17:31Z-
dc.date.available2008-09-22T16:17:31Z-
dc.date.issued1988-11-
dc.identifier.citationMonthly Notices Royal Astronomical Society, Vol. 235, pp. 221 – 228en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/3784-
dc.description.abstractHigh resolution observations of H-alpha 6563-A, forbidden O-III 5007 A, and forbidden N-II 6583-A emission lines in the bipolar planetary nebula NGC 2346 are presented. From the widths of the alpha and forbidden N-II lines, an ion temperature of 10,650 + or - 2950 K and a turbulent velocity 16 + or - 2 km/s are derived. Using the detailed radial velocity mapping done by Walsh (1983), a morphological model for the nebula is presented. It is suggested that the observed relative intensities of the approaching and receding components of emission lines in this nebula may very well be interpreted as due to the particular line-of-sight geometry in which the nebula is oriented.en
dc.language.isoenen
dc.publisherRoyal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1988MNRAS.235..221Aen
dc.subjectEmission Spectraen
dc.subjectH Alpha Lineen
dc.subjectLine Shapeen
dc.subjectPlanetary Nebulaeen
dc.subjectLine of Sighten
dc.subjectNitrogenen
dc.subjectOxygen Spectraen
dc.titleMorphology of the bipolar planetary nebula NGC 2346 from emission line profile studiesen
dc.typeArticleen
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