RMxAA

Revista Mexicana de Astronomía y Astrofísica

ISSN: 3061-8649
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Keywords

Galactic Structure
Kinematics
Solar Neighborhood
Stellar Systems
Superposition (Mathematics)
Computational Astrophysics
Distribution Functions
Gravitational Fields
Astrophysics
Solar Neighborhood:Kinematics

How to Cite

Superposición de sistemas estelares. II. (1987). Revista Mexicana De Astronomía Y Astrofísica, 15(1), 65-72. https://astronomia.unam.mx/journals/rmxaa/article/view/1987rmxaa..15...65r

Abstract

The author explains the kinematic behaviour of the stars of the solar neighbourhood supposing the superposition of two stellar populations. She considers both populations governed by a gravitational potential, stationary, with cylindrical symmetry and separable, which led her to impose conditions to the total distribution function. The superposition of the well-known stellar populations I and II, both governed by two simple distribution functions of Schwarzschild, explains satisfactorily the parameters observed in the solar neighbourhood.
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