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The two-body problem in the (truncated) PPN — Theory

✍ Scribed by M. Soffel; H. Ruder; M. Schneider


Publisher
Springer Netherlands
Year
1987
Tongue
English
Weight
509 KB
Volume
40
Category
Article
ISSN
1572-9478

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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