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Showing 1 to 2 of 2 for “"two-fluid treatment"”.
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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
… added in the post shock emission region. Our two-fluid^calculations are needed only in the small region bounded by M(, )>(, )1.2^M(,(CIRCLE)) and M(, )>(, )5 x 10('-3) M(,E), where M(,E) is the Eddington accretion rate^at which gravitational and radiation pressure forces balance (M(,E) = …
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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)