The effect of the particle number in the N body simulation for the aggregation formation of GMCS

Details The effect of the particle number in the N body simulation for the aggregation formation of GMCS The effect of the particle number in the N body simulation for the aggregation formation of GMCS

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002acasn..43..131z&link_type=abstract

Acta Astronomica Sinica, vol.43, no.2, p. 131-139

Astronomy and Astrophysics

Astronomy

Ism: Clouds, Ism: Evolution, Methods: N-Body Simulations

Scientific paper

In this paper, we study the effect of particle number in N body simulation for the aggregation formation of giant molecular cloud. The result shows that the averaged rate of the disrupted masses in GMCs where star birth occurs will keep the same in the models with different particle number if the mean density in the individual clouds with different masses is same, i.e., the ratio of the effective radii of collision for different model is proportional to the third root of corresponding masses in the individual clouds.

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