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A seminumerical 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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Keywords: Astrophysics; Radiating shells

Document Type: Research Article

Publication date: 2003-06-01

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