Published December 1986
| Version v1
Journal article
Study of the rotation velocity in the stellar system with axial symmetry
Creators
- 1. Universidad Politecnica de Cataluna, Barcelona (Spain). Dept. de Matematicas
- 2. Universidad de Barcelona (Spain). Dept. de Fisica de la Tierra y del Cosmos
Description
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 θ direction. (author)
Additional details
Additional titles
- Original title (Spanish)
- Estudio de la velocidad de rotacion en los sistemas estelares a simetria axial
Publishing Information
- Journal Title
- Rev. Mex. Astron. Astrof.
- Journal Volume
- 13
- Journal Issue
- 2
- Series
- Rev. Mex. Astron. Astrof.
- Journal Page Range
- 101-106
- ISSN
- 0185-1101
- CODEN
- RMAAD
INIS
- Country of Publication
- Mexico
- Country of Input or Organization
- Mexico
- INIS RN
- 19020386
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- AXIAL SYMMETRY; CHANDRASEKHAR THEORY; COSMOLOGICAL MODELS; GALACTIC EVOLUTION; GALAXIES; VELOCITY
- Descriptors DEC
- MATHEMATICAL MODELS; SYMMETRY