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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3625
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dc.contributor.authorBanerjee, D. P. K-
dc.contributor.authorAnandarao, B. G-
dc.contributor.authorJain, S. K-
dc.contributor.authorMallik, D. C. V-
dc.date.accessioned2008-09-15T14:44:50Z-
dc.date.available2008-09-15T14:44:50Z-
dc.date.issued1990-12-
dc.identifier.citationAstronomy and Astrophysics, Vol. 240, No. 1, pp. 137 - 141en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/3625-
dc.description.abstractHigh-resolution Fabry-Perot observations have been made to determine the velocity structure of five PNe and to subsequently relate the observations to the morphology of the objects. New kinematic data on one of these PNe, NGC 5882, are given and existing observations in other cases are supplemented. The effect of aperture size on expansion velocity in NGC 5882 is investigated. An attempt is made quantitatively to account for the unusual triple-peaked line profile observed in the bipolar nebula NGC 2818.en
dc.language.isoenen
dc.publisherThe European Southern Observatoryen
dc.relation.urihttp://cdsads.u-strasbg.fr/abs/1990A%26A...240..137Ben
dc.subjectAstronomical spectroscopyen
dc.subjectKinematicsen
dc.subjectMilky way galaxyen
dc.subjectPlanetary nebulaeen
dc.subjectRadial velocityen
dc.subjectFabry-Perot spectrometersen
dc.subjectLine spectraen
dc.subjectStellar structureen
dc.subjectVelocity distributionen
dc.titleKinematic studies of five galactic planetary nebulaeen
dc.typeArticleen
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