Modeling the Fourier-frequency resolved spectra of accreting black holes.

Details Modeling the Fourier-frequency resolved spectra of accreting black holes. Modeling the Fourier-frequency resolved spectra of accreting black holes.

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003head....7.1102z&link_type=abstract

American Astronomical Society, HEAD meeting #7, #11.02; Bulletin of the American Astronomical Society, Vol. 35, p.614

Astronomy and Astrophysics

Astronomy

Scientific paper

Fourier-frequency resolved spectra are energy spectra computed in a narrow range of Fourier frequency. They thus describe the energy spectrum of a component varying on a given timescale. They were computed from RXTE data of a few bright black hole X-ray binaries. I will present the Fourier spectra predicted by two models of accretion in low/hard state of accreting black holes: localized magnetic flares above an ionized disk, and a propagation model in the truncated disk/inner hot flow geometry. Spectra predicted from the former model are inconsistent with the observations, while the latter model can reproduce the data.

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