Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2646
Title: Flat rotation curves: A result of the helical inverse cascade in turbulent media?
Authors: Prabhu, R. D
Krishan, V
Keywords: Curves (Geometry);Galactic Structure;Galaxies;Gravitational Fields;Rotation;Turbulence Models;Angular Velocity;Hydrodynamics;Numerical Analysis;Radii;Turbulent Flow
Issue Date: Jun-1994
Publisher: The American Physical Society
Citation: Astrophysical Journal, Vol. 428, No. 2, Part. 1, pp. 483 - 492
Abstract: We 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.
URI: http://hdl.handle.net/2248/2646
ISSN: 0004-637X
???metadata.dc.relation.uri???: http://adsabs.harvard.edu/abs/1994ApJ...428..483P
Appears in Collections:IIAP Publications

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