Trajectories of the local centroids in a two-component stellar system near the sun

Details Trajectories of the local centroids in a two-component stellar system near the sun Trajectories of the local centroids in a two-component stellar system near the sun

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.170..197c&link_type=abstract

(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640

Astronomy and Astrophysics

Astrophysics

2

Centroids, Solar Neighborhood, Stellar Systems, Trajectory Analysis, Kinematic Equations, Velocity Distribution

Scientific paper

In a stellar system in nonsteady states and according to Chandrasekhar's axially symmetric model, the general trajectory of a local centroid is determined. In the neighborhood of the sun, a two-component stellar system is adopted to explain the kinematic behavior of the stellar samples. Depending on the kinematic parameters of each subsystem, the trajectories of every local subcentroid are shown.

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