The evolution of self-gravitating clusters of gas-dust nebulae participating in planetary body accumulation

Details The evolution of self-gravitating clusters of gas-dust nebulae participating in planetary body accumulation The evolution of self-gravitating clusters of gas-dust nebulae participating in planetary body accumulation

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989avest..23...14m&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 23, Jan.-Mar. 1989, p. 14-26. In Russian.

Statistics

Computation

Computational Astrophysics, Cosmic Dust, Cosmic Gases, Nebulae, Planetary Evolution, Protoplanets, Cauchy Problem, Density Distribution, Gravitational Effects, Mathematical Models, Pressure Distribution, Temperature Distribution

Scientific paper

A mathematical model for the evolution of self-gravitating gas-dust clusters is presented. A method of two-scale expansion to a set of hydrodynamic and thermodynamic equations describing the behavior of the self-gravitating gas-dust clusters is used. The dependence of the pressure and temperature distribution functions on the mass and characteristic density values and the typical course of cluster evolution is analyzed.

Affiliated with

Also associated with

No associations

Rating

The evolution of self-gravitating clusters of gas-dust nebulae participating in planetary body accumulation does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The evolution of self-gravitating clusters of gas-dust nebulae participating in planetary body accumulation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The evolution of self-gravitating clusters of gas-dust nebulae participating in planetary body accumulation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1801701