We present preliminary results of the hydrodynamical simulations of the collapse of a protogalaxy up to star formation.
A Multifluid Hydrodynamical Radiative Model for the Evolution of a Spherical Protogalaxy / CAPUZZO DOLCETTA, R.A., A., D.F., A. B., M.. - STAMPA. - (1990), pp. 303-317. (Physcal Processes in fragmentation and Star Formation Monteporzio catone, Roma, Italy June 5-1-, 1989).
A Multifluid Hydrodynamical Radiative Model for the Evolution of a Spherical Protogalaxy
CAPUZZO DOLCETTA, Roberto Angelo;
1990
Abstract
We present preliminary results of the hydrodynamical simulations of the collapse of a protogalaxy up to star formation.File allegati a questo prodotto
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