Hostname: page-component-848d4c4894-wg55d Total loading time: 0 Render date: 2024-05-21T03:21:43.349Z Has data issue: false hasContentIssue false
  • English
  • Français

Fragmentation of Isothermal Gas Clouds

Published online by Cambridge University Press:  14 August 2015

R. A. Gingold  and
J. J. Monaghan
R. A. Gingold
Affiliation:
Department of Mathematics, Monash University, Australia
J. J. Monaghan
Affiliation:
Department of Mathematics, Monash University, Australia

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

An analysis of the collapse and fission of the isothermal gas cloud examined by Boss and Bodenheimer (BB, 1979) has been made using SPH (Lucy 1977, Gingold and Monaghan 1977, 1978). While SPH is not as effective as finite difference methods for problems with spherical symmetry, it has the advantage in fragmentation problems that the description of the fragments is independent of their position and orientation. Furthermore, the SPH algorithm has been tested by applying it to non axisymmetric problems for which accurate solutions are known as well as spherically and axially symmetric problems.

Type
Session 2: Pre-Main-Sequence Evolution and Formation of Binary Stars
Information
Symposium - International Astronomical Union , Volume 93: Fundamental Problems in the Theory of Stellar Evolution , 1981 , pp. 107 - 108
Copyright
Copyright © Reidel 1981 

References

Boss, A.P. and Bodenheimer, P.: 1979, Astrophys. J., 234, pp.289–295.CrossRefGoogle Scholar
Gingold, R. and Monaghan, J.: 1977, Mon. Not. Roy. Astr. Soc. 181, pp.375–389.CrossRefGoogle Scholar
Gingold, R. and Monaghan, J.: 1978, Mon. Not. Roy. Astr. Soc. 184,pp.481–499.CrossRefGoogle Scholar
Lucy, L.B.: 1977, Astron. J., 82, pp.1013–1024.CrossRefGoogle Scholar