Abstract
In a previous series of papers relating to the Combined Gravitational Action (CGA), we have exclusively studied orbital motion without spin. In the present paper we apply CGA to any self-rotating material body, i.e., an axially spinning massive object, which itself may be locally seen as a gravitorotational source because it is capable of generating the gravitorotational acceleration field, which seems to be unknown to previously existing theories of gravity. The consequences of such an acceleration field are very interesting, particularly for Sun and Compact Stellar Objects.
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