Collapse and fragmentation of isothermal gas clouds

Details Collapse and fragmentation of isothermal gas clouds Collapse and fragmentation of isothermal gas clouds

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.194..201w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 194, Jan. 1981, p. 201-218.

Other

52

Gravitational Collapse, Interstellar Gas, Isothermal Processes, Molecular Clouds, Molecular Gases, Boundary Value Problems, Equations Of Motion, Finite Difference Theory, Fragments, Monte Carlo Method, Numerical Integration

Scientific paper

An initial boundary value problem for the three-dimensional motion of a collapsing, isothermal gas cloud is solved using a numerical method. The method is based on the Monte-Carlo scheme, with the equations integrated using a high order N-body code, allowing individual time-steps for each element. The results show that the method is capable of following the growth of instabilities but further work is necessary.

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