Browse Dept. of Physics by Subject "accreting non-magnetic degenerate dwarfs"
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(1978)X radiation from degenerate stars is produced by the impact of accreting matter with the stellar surface. The resulting X-ray and UV spectrum gives vital clues about the nature of the underlying star and the extreme ...
X and UV radiation from accreting non-magnetic degenerate dwarfs: A two-fluid treatment of the emission region and the effects of steady nuclear burning (1981)