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Newtonian gravitational field theory: Two-body problem

✍ Scribed by Solomon L. Schwebel


Publisher
Springer
Year
1971
Tongue
English
Weight
299 KB
Volume
4
Category
Article
ISSN
0020-7748

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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