Abstract
A semi-numeric method was used to study the evolution of a general-relativistic radiating shell in its Post-Newtonian and Newtonian approximations. The solutions, where the main parameters are given reasonable values, show that a relativistic effect can be found in X-ray-burster-like objects.
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Santoro, F., Aquilano, R. & Ibaceta, D. Contraction of Radiating Shell in Classical and Post-NewtonianApproximation. Astrophysics and Space Science 268, 469–474 (1999). https://doi.org/10.1023/A:1002035223803
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DOI: https://doi.org/10.1023/A:1002035223803