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of the research: Symbiotic stars are interacting binaries with very long orbital periods (on the order of years). They consist of a red giant that is losing some of its mass and a white dwarf that is accreting it
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the formation of the Oort cloud in its birth star cluster. In more detail, we will solve open questions of this process using numerical simulations with respect of recent observations. Among answers on various
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and their development, and thus also their integration into the evolution of other stars and stellar systems. Objectives: For selected fast and slow novae, determine the basic physical parameters
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