Predictions for Fourier-resolved X-ray spectroscopy from the model of magnetic flare avalances above an accretion disk with a hot ionized skin

Details Predictions for Fourier-resolved X-ray spectroscopy from the model of magnetic flare avalances above an accretion disk with a hot ionized skin Predictions for Fourier-resolved X-ray spectroscopy from the model of magnetic flare avalances above an accretion disk with a hot ionized skin

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002bhty.confe..33z&link_type=multimedia

Presented at the KITP Conference: Black Holes: Theory Confronts Reality, Three Years Later, Feb 25, 2002, Kavli Institute for Th

Physics

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