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. Understanding the solid phases of ices is crucial for studying how their molecular structures influence radiation-driven astrochemical processes (e.g. phase transition, ice compaction, radiolytic decay
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: The nova phenomenon is the result of the sudden thermonuclear fusion of hydrogen into helium in the surface layer of a white dwarf (WD). The fuel for this process is hydrogen material that is deposited
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of their research. Objectives: The aim of the PhD thesis is to determine the basic physical parameters of the BF Cyg radiation regions (temperatures, radii, luminosities, emission volume, mass-loss rate from the
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