N-body simulation of Giant Molecular Clouds in a galaxy

Details N-body simulation of Giant Molecular Clouds in a galaxy N-body simulation of Giant Molecular Clouds in a galaxy

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.118..463t&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

Astronomical Models, Many Body Problem, Milky Way Galaxy, Molecular Clouds, Gravitational Effects, Random Processes, Velocity Distribution

Scientific paper

An N-body simulation of Giant Molecular Clouds in a model galaxy was
made. It was confirmed that their random motion is generated and
accelerated by purely gravitational interaction among them over some 10
to 100 million years. The results of the present simulation agree well
with those of the previous theoretical calculation by Fukunaga (1984).

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