The effect of the radiation-pressure in the problem of the two bodies is analysed. It is found that such an effect is the same as that of reducing the stellar mass, m, by the factor p (0 5 p 5 1 ) . The case p < 0 leads to stellar instability and, consequently, it is not considered here. The problem
β¦ LIBER β¦
Non-Riemann geometrizable effects in the gravitational one-body problem
β Scribed by I. W. Roxburgh; R. K. Tavakol
- Publisher
- Springer US
- Year
- 1979
- Tongue
- English
- Weight
- 243 KB
- Volume
- 10
- Category
- Article
- ISSN
- 0001-7701
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Photoβgravitational effects in the twoβb
β
I. Todoran; R. Roman
π
Article
π
1993
π
John Wiley and Sons
π
English
β 174 KB
π 1 views
On the Gravitational Two-Body Problem in
β
Dr. G. N. Afanasiev; R. A. Asanov
π
Article
π
1981
π
John Wiley and Sons
π
English
β 566 KB
Effects of non-homogeneity on the stress
β
J. G. Chakravorty; Y. De
π
Article
π
1971
π
Springer
π
English
β 271 KB
Effects of non-homogeneity on the stress
β
A. Mukhopadhyay
π
Article
π
1974
π
Springer
π
English
β 307 KB
Effect of the potential field on non-Fic
β
Han-Taw Chen; Kuo-Chi Liu
π
Article
π
2003
π
Elsevier Science
π
English
β 202 KB
The present study applies a hybrid numerical method to investigate the effect of a potential field on one-dimensional non-Fickian diffusion problems in a sphere. This hybrid numerical scheme involves the Laplace transform technique and the control volume method in conjunction with the suitable hyper
The effect of a non-uniform internal pre
β
E. Smith
π
Article
π
1966
π
Elsevier Science
π
English
β 592 KB