Orbits of Stars in a Model with Three First Integrals

Details Orbits of Stars in a Model with Three First Integrals Orbits of Stars in a Model with Three First Integrals

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990rmxaa..21..259c&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, 21, 259

Astronomy and Astrophysics

Astronomy

1

Scientific paper

RESUNEN. Se apliCa una forma integrable del potencial de la Galaxia para describir la variaci6n de los pericentros y apoCentros de las 6rbitas de las estrellas de acuerdo C0fl SuS velocidades en el entorno solar. Conio ejemplo, se presenta Un estudio mas detallado de la 6rbita del 501. A8STRACT. An integrable form of the potential of the Galaxy is applied to describe the variation of the pericentres and the apocentres of the orbits of stars in accordance with their velocities in the solar neighbourhood. As an example, a more detailed study of the orbit of the Sun is presented. Key words: DYNAMICS -- GALAXY-STRUCTURE

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