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Fast Spectral Variability in the X-ray Emission of Accreting Black Holes (Hardcover, 2015 ed.)
Loot Price: R3,481
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Fast Spectral Variability in the X-ray Emission of Accreting Black Holes (Hardcover, 2015 ed.)
Series: Springer Theses
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This thesis brings together the various techniques of X-ray
spectral analysis in order to examine the properties of black holes
that vary in mass by several orders of magnitude. In all these
systems it is widely accepted that the X-ray emission is produced
by Compton up-scattering of lower energy seed photons in a hot
corona or accretion flow, and here these processes are examined
through a study of the X-ray spectral variability of each source. A
new technique is introduced, in which models are fitted to over 2
million X-ray spectra on time-scales as short as 16 ms, and
subsequently it is shown that the nature of the correlation between
intensity and spectral index is strongly dependent upon the
spectral state of the black hole. Finally, the results of an
extensive survey of nearby galactic nuclei using the Chandra X-ray
telescope are presented in the form of images and spectra, and
these results are used along with data from the literature to
search for Compton-thick nuclei.
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