Spatial And Spectral Anomalies In The Soft X Ray Background

Author: Pieter A. de Korte
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ISBN:
File Size: 59,48 MB
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Small Scale Spatial Fluctuations In The Soft X Ray Background

Author: Kip D. Kuntz
Editor:
ISBN:
File Size: 47,28 MB
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X Ray Astronomy In The 1980 S

Author: Stephen S. Holt
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ISBN:
File Size: 75,41 MB
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Spatial Structure Of The Diffuse Soft X Ray Background

Author: David Nelson Burrows
Editor:
ISBN:
File Size: 47,41 MB
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Observations Of The Diffuse Soft X Ray Background From 0 07 To 1 0 Kev

Author: Jeffrey Joseph Bloch
Editor:
ISBN:
File Size: 38,74 MB
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The Study Of The Diffuse X Ray Background Between 150 Ev 280 Ev With The Diffuse X Ray Spectrometer Dxs

Author: Jeffrey Paul Morgenthaler
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ISBN:
File Size: 46,17 MB
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Nuclear Science Abstracts

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File Size: 70,43 MB
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Soviet Life

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File Size: 29,21 MB
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X Ray Detector Physics And Applications

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File Size: 25,43 MB
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Frontiers Of X Ray Astronomy

Author: Yasuo Tanaka
Editor:
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File Size: 14,32 MB
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The X Ray Background

Author: Xavier Barcons
Editor: Cambridge University Press
ISBN: 9780521416511
File Size: 35,76 MB
Format: PDF
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A review of the current observational knowledge and understanding of the cosmic X-ray background.

Physics Briefs

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File Size: 36,76 MB
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Euv X Ray And Gamma Ray Instrumentation For Astronomy

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File Size: 71,17 MB
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Advances In X Ray Analysis

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File Size: 11,44 MB
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X Ray Clusters Of Galaxies

Author: John David McKee
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File Size: 25,18 MB
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X Ray Astronomy And Related Topics

Author: R. D. Andresen
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File Size: 21,63 MB
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Soviet Physics Uspekhi

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File Size: 21,33 MB
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Government Reports Announcements Index

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File Size: 34,10 MB
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Dxs The Diffuse X Ray Spectrometer

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File Size: 49,95 MB
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Suzaku Studies Of White Dwarf Stars And The Galactic X Ray Background Emission

Author: Takayuki Yuasa
Editor: Springer Science & Business Media
ISBN: 4431542191
File Size: 41,81 MB
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This thesis presents a study of the origin of an apparently extended X-ray emission associated with the Galactic ridge. The study was carried out with broadband spectra obtained from mapping observations in the Galactic bulge region conducted in 2005–2010 by the Suzaku space X-ray observatory. The spectra were analyzed with a newly constructed X-ray spectral model of an accreting white dwarf binary that is one of the proposed candidate stars for the origin of the Galactic ridge emission in the higher energy band. Fitting of the observed Galactic ridge spectra with the model showed that there is another spectral component that fills the gap between the observed X-ray flux and the component expected from the accreting white dwarf spectral model in the lower energy band. This additional soft spectral component was nicely explained by an X-ray spectral model of normal stars. The result, together with previously reported high-resolution imaging results, strongly supports the idea that the Galactic ridge X-ray emission is an assembly of dim, discrete X-ray point sources.