Physics
Scientist
Roma, Osservatorio Astronomico; Roma, Università, Rome, Italy
Roma, Universita, Rome, Italy
Axisymmetric gravitational collapse of an isothermal rotating interstellar gas cloud. I - A semi-analytical approach
Axisymmetric gravitational collapse of rotating interstellar gas clouds
Evolution of weak discontinuity waves in self-similar flows and formation of secondary shocks - The 'point explosion model'
Molecular Ratios Sensitive to Elemental Abundances
On the mass distribution law of systems of protocluster fragments
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