A New Comptonization Model for Weakly Magnetized Accreting NS LMXBs

Details A New Comptonization Model for Weakly Magnetized Accreting NS LMXBs A New Comptonization Model for Weakly Magnetized Accreting NS LMXBs

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1126..316p&link_type=abstract

SIMBOL-X: FOCUSING ON THE HARD X-RAY UNIVERSE: Proceedings of the 2nd International Simbol-X Symposium. AIP Conference Proceedi

Physics

X-Ray Sources, X-Ray Bursts, Pulsars, Spectroscopy And Spectrophotometry, Infall, Accretion, And Accretion Disks

Scientific paper

We have developed a new Comptonization model to propose, for the first
time, a self consistent physical interpretation of the complex spectral
evolution seen in NS LMXBs. The model and its application to LMXBs are
presented and compared to the Simbol-X expected capabilities.

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