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Study of the rotation velocity in the stellar system with axial symmetry

Author
Sanz, J.; Català, M.
Type of activity
Journal article
Journal
Revista mexicana astronomía y astrofísica
Date of publication
1986-11-10
Volume
13
Number
2
First page
101
Last page
106
Repository
http://hdl.handle.net/2117/99990 Open in new window
Abstract
This paper contains the calculation of the tangential component of the velocity for a model of galaxy with axial symmetry, non stationary state and equatorial symmetry plane, from the postulates and fundamental equations of Chandrasekhar theory, that shows a shift of the maximum for different values of the Z coordinate and the ¿ direction.
Citation
Sanz, J., Català, M. Study of the rotation velocity in the stellar system with axial symmetry. "Revista mexicana astronomía y astrofísica", 10 Novembre 1986, vol. 13, núm. 2, p. 101-106.
Keywords
stellar dynamics, stellar systems
Group of research
gAGE - Research Group of Astronomy and Geomatics

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