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Showing 1 to 4 of 4 for “"accreting non-magnetic degenerate dwarfs"”.
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X and Ultraviolet Radiation From Accreting Non-Magnetic Degenerate Dwarfs
Made available in DSpace on 2015-05-13T15:22:13Z (GMT). No. of bitstreams: 2 license.txt: 4848 bytes, checksum: 96035ab3f5e1c23cc7138a224ce498bd (MD5) 7820984.PDF: 5219161 bytes, checksum: 06e98661cbf36ae706c03af2d786212a (MD5) Previous issue date: 1978
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X and UV radiation from accreting non-magnetic degenerate dwarfs
"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 conditions of temperature and magnetic field strength that may exist in the …
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X and Ultraviolet Radiation From Accreting Non-Magnetic Degenerate Dwarfs: A Two-Fluid Treatment of the Emission Region and the Effects of Steady Nuclear Burning
The first main chapter is a report of the results of calculations which^allow the temperatures of the electrons and the ions to differ and which^include electron thermal conduction. The calculation is done in spherical^geometry, with cooling by bremsstrahlung and cooling by the inverse^Compton …
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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
Submitted by Carolyn Mead (cmead2@illinois.edu) on 2011-06-16T16:21:56Z No. of bitstreams: 1 1981_weast.pdf: 3157656 bytes, checksum: c43d64a0b86da434a1750cf61a63b211 (MD5)