Superposition of stellar systems. II

Details Superposition of stellar systems. II Superposition of stellar systems. II

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987rmxaa..15...65r&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica (ISSN 0185-1101), vol. 15, Dec. 1987, p. 65-72. In Spanish.

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2

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

Scientific paper

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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