A method for the calculation of axially symmetric dynamical systems

Details A method for the calculation of axially symmetric dynamical systems A method for the calculation of axially symmetric dynamical systems

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....47..407f&link_type=abstract

Astronomy and Astrophysics, vol. 47, no. 3, Mar. 1976, p. 407-412. Research supported by the Deutsche Forschungsgemeinschaft.

Other

13

Axisymmetric Bodies, Computer Techniques, Gravitational Collapse, Protostars, Stellar Evolution, Stellar Structure, Angular Momentum, Finite Difference Theory, Isothermal Processes, Legendre Functions, Stellar Rotation, Velocity Distribution

Scientific paper

A two-dimensional computer code is described which is suitable for hydrodynamic self-gravitating systems with axial symmetry. While the radial coordinate is treated by a difference scheme, the angular dependence of every function is expanded into Legendre polynomials. The expansion coefficients are computed using a conventional Henyey scheme. The results of test computations for the collapse of rotating isothermal protostellar clouds with two different values of angular momentum are presented.

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