Hostname: page-component-cd9895bd7-p9bg8 Total loading time: 0 Render date: 2024-12-28T18:14:05.541Z Has data issue: false hasContentIssue false
  • English
  • Français

A hydrodynamical study of fragmenting gas clouds

Published online by Cambridge University Press:  03 August 2017

Joe Monaghan  and
John Lattanzio
Joe Monaghan
Affiliation:
Department of Mathematics, Monash University, Clayton, Victoria, 3168, AUSTRALIA
John Lattanzio
Affiliation:
Department of Mathematics, Monash University, Clayton, Victoria, 3168, AUSTRALIA Institute of Geophysics and Planetary Physics, L-413, L.L.N.L., P.O. Box 808, Livermore, Ca., 94550, USA

Abstract

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.

We present 3-D hydrodynamical calculations of collapsing rotating gas clouds, with molecular cooling. We find that cooling significantly inreases the number of fragments.

Type
Poster Sessions
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 464 - 465
Copyright
Copyright © Kluwer 1991 

References

Hollenbach, D. and McKee, C., 1979, Astrophys. J. Suppl. Ser., 41, 555.CrossRefGoogle Scholar
Monaghan, J. J., and Lattanzio, J. C., 1990, Astrophys. J., submitted.Google Scholar
Adams, F. C., Ruden, S. P., and Shu, F. H., 1989, Astrophys. J., 347, 959.Google Scholar
Welch, W. J., et al, 1987, Science, 238, 1550.CrossRefGoogle Scholar