Kinematic constraints between stellar systems in superposition

Details Kinematic constraints between stellar systems in superposition Kinematic constraints between stellar systems in superposition

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.170..337c&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

Chandrasekhar Equation, Kinematic Equations, Potential Fields, Stellar Systems, Unsteady State, Astronomical Models, Axisymmetric Bodies, Stellar Motions, Velocity Distribution

Scientific paper

Some kinematic consequences of a superposition of two stellar systems are studied. Chandrasekhar's axially-symmetric model has been adopted for each one of the subsystems. The solution of Chandrasekhar's equations provides us with a potential function, which must be shared by both stellar subsystems and, thus, some relationships between the kinematic parameters of both subsystems are obtained. In the case of a stationary potential function the whole set of second-order centered moments may be explained.

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