Problems on gravitational collapse of interstellar gas clouds. I Numerical integration of the equations of hydrodynamics - The case of spherical symmetry

Details Problems on gravitational collapse of interstellar gas clouds. I Numerical integration of the equations of hydrodynamics - The case of spherical symmetry Problems on gravitational collapse of interstellar gas clouds. I Numerical integration of the equations of hydrodynamics - The case of spherical symmetry

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975mmsai..46..313f&link_type=gif

Società Astronomica Italiana, Memorie, vol. 46, Aug. 1975, p. 313-339. Research supported by the Consiglio Nazionale delle Rice

Astronomy and Astrophysics

Astronomy

5

Gas Dynamics, Gravitational Collapse, Hydrodynamic Equations, Interstellar Gas, Numerical Integration, Equations Of Motion, Gas Heating, Graphs (Charts), Luminous Intensity, Pressure Distribution, Radial Velocity, Temperature Gradients, Thermodynamic Properties

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