EXOSAT light curve of AM HerAM Her displays a strong variable soft X-ray flux in this EXOSAT observation which is anticorrelated with the hard (higher temperature) X-rays. The eclipse of the soft X-rays for a large fraction of the 3.1 hour binary cycle is due to the occultation of the X-ray emitting pole cap by the white dwarf star itself. The hard X-rays are produced by a shock within the accretion column and are only modulated when the column cuts across our line of sight. Diagrams courtesy of Julian Osborne, EXOSAT Observatory, taken from Figure 10-4a in Charles and Seward.
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HEASARC Home | Observatories | Archive | Calibration | Software | Tools | Students/Teachers/Public Last modified: Thursday, 26-Jun-2003 13:48:44 EDT HEASARC Staff Scientist Position - Applications are now being accepted for a Staff Scientist with significant experience and interest in the technical aspects of astrophysics research, to work in the High Energy Astrophysics Science Archive Research Center (HEASARC) at NASA Goddard Space Flight Center (GSFC) in Greenbelt, MD. Refer to the AAS Job register for full details. |