Rashed Omari, H. Y., and et al., Dec. 2008,
Magnitudes of bremsstrahlung and cyclotron cooling from on-axis accretion shocks onto AM-Her systems,
Jordan Journal of Physics, vol. 1, no. 2, pp. 79-87.
The article presents a calculation to relative phases and relative magnitudes for bremsstrahlung and cyclotron emissions from radiative accretion shocks onto binary Magnetic CVs (AM-Her systems). The calculation is carried out for a 0.3 solar mass white dwarf primary star, having a field B*=30MG, and accretion rate of Lacc =3.2x10-3 LEdd. Here LEdd is the Eddington accretion luminosity. Individual on-axis accretion funnels are being investigated corresponding to large radii at which field lines strike the equatorial plane (a0=req/R*= 500, 300, 200, 150, 100, and 80). Results show a relatively low level cyclotron cooling, and thus permit decoupling.
http://journals.yu.edu.jo/jjp/JJPIssues/Vol1No2_2008PDF/3-Magnitudes%20of%20Bremsstrahlung,%20Omary%20et%20al2.pdf
