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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2646
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dc.contributor.authorPrabhu, R. D-
dc.contributor.authorKrishan, V-
dc.date.accessioned2008-07-14T05:43:37Z-
dc.date.available2008-07-14T05:43:37Z-
dc.date.issued1994-06-
dc.identifier.citationAstrophysical Journal, Vol. 428, No. 2, Part. 1, pp. 483 - 492en
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2248/2646-
dc.description.abstractWe have modeled the rotation curves of 21 galaxies observed by Amram et al. (1992), by combining the effects of rigid rotation, gravity, and turbulence. The main motivation behind such modeling is to study the formation of coherent structures in turbulent media and explore its role in the large-scale structures of the universe. The values of the parameters such as mass, turbulent velocity, and angular velocity derived from the rotation curve fits are in good agreement with those derived from the prevalent models.en
dc.format.extent937053 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe American Physical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1994ApJ...428..483Pen
dc.subjectCurves (Geometry)en
dc.subjectGalactic Structureen
dc.subjectGalaxiesen
dc.subjectGravitational Fieldsen
dc.subjectRotationen
dc.subjectTurbulence Modelsen
dc.subjectAngular Velocityen
dc.subjectHydrodynamicsen
dc.subjectNumerical Analysisen
dc.subjectRadiien
dc.subjectTurbulent Flowen
dc.titleFlat rotation curves: A result of the helical inverse cascade in turbulent media?en
dc.typeArticleen
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