Formation and evolution of rings in disk-shaped protostellar clouds

Details Formation and evolution of rings in disk-shaped protostellar clouds Formation and evolution of rings in disk-shaped protostellar clouds

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984acasn..25..156l&link_type=abstract

(Acta Astronomica Sinica, vol. 25, no. 2, 1984, p. 156-167) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 8, Dec. 19

Statistics

Computation

Clouds, Computational Astrophysics, Protostars, Stellar Evolution, Density Distribution, Ring Structures

Scientific paper

Numerical simulation of the evolution of a disc-like system of protostellar clouds is made by means of N gravitating bodies. It is shown that the ring structure is physically present in the course of the gravitational collapse, that the ring structure represents only one stage of the cloud's evolution, and that it will eventually break up into new structures.

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