Titlebook: High Energy Astrophysics; Supernovae, Remnants Gerhard B?rner Conference proceedings 1988 Springer-Verlag Berlin Heidelberg 1988 Accretion.

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Line Emission from Magnetized Neutron Stars and Electron Cyclotron Maser Instabilityow beam velocity distributions. The growth rates increase proportionally with the electron density in the accretion column, and vary rapidly with emission angle. The observations about the intensity and the energy of emission line correlated with Her X-1 pulse phase have also been explained.

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