KIAM Main page Web Library  •  Publication Searh  Русский 

KIAM Preprint № 109, Moscow, 2014
Authors: Strakhovskaya L. G.
Numerical model of the cooling gravitating gas disk
Evolution of the gas cloud, rotating around the gravitating center, is investigated. The influence of self-gravitation and cooling of disk on the formation of its configuration is studied. The influence of gravity of central object and self-gravitation leads to the intensive compression of cloud, an increase in the density and temperature. Because of an increase in the temperature the pressure, which counteracts compression, grows, and density gradually is reduced. The calculation of the simple law of cooling reduces temperature, density decreases less. The possibility of the disk fragmentation appears.
gas disk, self-gravitation, fragmentation, cooling
Publication language: russian,  pages: 16
Research direction:
Mathematical modelling in actual problems of science and technics
Russian source text:
List of publications citation:
Export link to publication in format:   RIS    BibTeX
View statistics (updated once a day)
over the last 30 days — 0 (-4), total hit from 01.09.2019 — 29
About authors:
  • Strakhovskaya Liudmila Glebovna,  KIAM RAS