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Fast spectral variability in the x-r...
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Skipper, Chris.
Fast spectral variability in the x-ray emission of accreting black holes[electronic resource] /
紀錄類型:
書目-語言資料,印刷品 : Monograph/item
杜威分類號:
522.6863
書名/作者:
Fast spectral variability in the x-ray emission of accreting black holes/ by Chris Skipper.
作者:
Skipper, Chris.
出版者:
Cham : : Springer International Publishing :, 2015.
面頁冊數:
xxxiii, 150 p. : : ill., digital ;; 24 cm.
Contained By:
Springer eBooks
標題:
X-ray astronomy.
標題:
Accretion (Astrophysics)
標題:
Black holes (Astronomy)
標題:
Astrophysics.
標題:
Physics.
標題:
Astronomy, Observations and Techniques.
ISBN:
9783319095875 (electronic bk.)
ISBN:
9783319095868 (paper)
內容註:
Declaration of Authorship -- Acknowledgements -- Introduction -- AGN: Absorption, spectral classification and the optical emission lines -- Very Fast X-ray Spectral Variability in Cygnus X-1 -- The mE relationship in XRBs and AGN -- Conclusions -- Spectra of Compton-thick AGN -- Spectra of Compton-thin AGN -- References.
摘要、提要註:
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.
電子資源:
http://dx.doi.org/10.1007/978-3-319-09587-5
Fast spectral variability in the x-ray emission of accreting black holes[electronic resource] /
Skipper, Chris.
Fast spectral variability in the x-ray emission of accreting black holes
[electronic resource] /by Chris Skipper. - Cham :Springer International Publishing :2015. - xxxiii, 150 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..
Declaration of Authorship -- Acknowledgements -- Introduction -- AGN: Absorption, spectral classification and the optical emission lines -- Very Fast X-ray Spectral Variability in Cygnus X-1 -- The mE relationship in XRBs and AGN -- Conclusions -- Spectra of Compton-thick AGN -- Spectra of Compton-thin AGN -- References.
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.
ISBN: 9783319095875 (electronic bk.)
Standard No.: 10.1007/978-3-319-09587-5doiSubjects--Topical Terms:
602964
X-ray astronomy.
LC Class. No.: QB472
Dewey Class. No.: 522.6863
Fast spectral variability in the x-ray emission of accreting black holes[electronic resource] /
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Declaration of Authorship -- Acknowledgements -- Introduction -- AGN: Absorption, spectral classification and the optical emission lines -- Very Fast X-ray Spectral Variability in Cygnus X-1 -- The mE relationship in XRBs and AGN -- Conclusions -- Spectra of Compton-thick AGN -- Spectra of Compton-thin AGN -- References.
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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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