The evolution of the different chemical species are followed in a model of contracting interstellar cloud. The central density increases from n = 10 cme3 diffuse initial cloud model to a dense cloud with central density number of n 1 lo5 cmA3 after a time of 1.2 x lo7 yr. A network of 622 reactions
โฆ LIBER โฆ
Contraction models for the evolution of Jupiter
โ Scribed by Peter Bodenheimer
- Publisher
- Elsevier Science
- Year
- 1976
- Tongue
- English
- Weight
- 547 KB
- Volume
- 29
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
The chemical evolution in a model of con
โ
M. Y. Amin; M. S. El-Nawawy
๐
Article
๐
1997
๐
Springer Netherlands
๐
English
โ 741 KB
Calculations of the early evolution of J
โ
Peter Bodenheimer
๐
Article
๐
1974
๐
Elsevier Science
๐
English
โ 601 KB
Implications of Jupiter's early contract
โ
James B. Pollack; Ray T. Reynolds
๐
Article
๐
1974
๐
Elsevier Science
๐
English
โ 482 KB
Young Jupiters are faint: new models of
โ
J. J. Fortney; M. S. Marley; O. Hubickyj; P. Bodenheimer; J. J. Lissauer
๐
Article
๐
2005
๐
John Wiley and Sons
๐
English
โ 210 KB
The evolution of charged particles in a
โ
M. S. El-Nawawy; M. Y. Amin
๐
Article
๐
1997
๐
Springer Netherlands
๐
English
โ 561 KB
The evolution of the charged particles are followed during contraction of a model of an interstellar cloud, with initial density number of n = 10 cmV3. The contraction is followed up to density increase by five orders of magnitude. Special care is given to the details of the negative ions. In addit
Two models for the evolution of polygyny
โ
Stuart A. Altmann; Stephen S. Wagner; Sarah Lenington
๐
Article
๐
1977
๐
Springer
๐
English
โ 951 KB