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024 7 $a10.1007/978-4-431-54219-3
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035   $a(EBL)1083421
035   $a(OCoLC)826853750
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035   $a(PQKBManifestationID)11450885
035   $a(PQKBTitleCode)TC0000854868
035   $a(PQKBWorkID)10911488
035   $a(PQKB)10220046
035   $a(DE-He213)978-4-431-54219-3
035   $a(MiAaPQ)EBC1083421
035   $a(PPN)168332612
035   $a(EXLCZ)992670000000328419
100   $a20130125d2013      u|             0
101 0 $aeng
135   $aur|n|---|||||
181   $ctxt
182   $cc
183   $acr
200 10$aSuzaku Studies of White Dwarf Stars and the Galactic X-ray Background Emission$b[electronic resource] /$fby Takayuki Yuasa
205   $a1st ed. 2013.
210  1$aTokyo :$cSpringer Japan :$cImprint: Springer,$d2013.
215   $a1 online resource (162 p.)
225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053
300   $aDescription based upon print version of record.
311   $a4-431-54717-7 
311   $a4-431-54218-3 
320   $aIncludes bibliographical references.
327   $aReview of the Galactic X-ray Background Emission and White Dwarf Binaries -- Constructing an X-ray Model of Accreting White Dwarf Binaries -- Instrumentation -- Estimating the Masses of White Dwarfs in Magnetic Cataclysmic Variables -- Decomposing the Galactic Ridge X-ray Emission.
330   $aThis thesis presents a study of the origin of an apparently extended X-ray emission associated with the Galactic ridge. The study was carried out with broadband spectra obtained from mapping observations in the Galactic bulge region conducted in 2005?2010 by the Suzaku space X-ray observatory. The spectra were analyzed with a newly constructed X-ray spectral model of an accreting white dwarf binary that is one of the proposed candidate stars for the origin of the Galactic ridge emission in the higher energy band. Fitting of the observed Galactic ridge spectra with the model showed that there is another spectral component that fills the gap between the observed X-ray flux and the component expected from the accreting white dwarf spectral model in the lower energy band. This additional soft spectral component was nicely explained by an X-ray spectral model of normal stars. The result, together with previously reported high-resolution imaging results, strongly supports the idea that the Galactic ridge X-ray emission is an assembly of dim, discrete X-ray point sources.
410  0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053
606   $aObservations, Astronomical
606   $aAstronomy?Observations
606   $aPhysical measurements
606   $aMeasurement   
606   $aAstronomy, Observations and Techniques$3https://scigraph.springernature.com/ontologies/product-market-codes/P22014
606   $aMeasurement Science and Instrumentation$3https://scigraph.springernature.com/ontologies/product-market-codes/P31040
615  0$aObservations, Astronomical.
615  0$aAstronomy?Observations.
615  0$aPhysical measurements.
615  0$aMeasurement   .
615 14$aAstronomy, Observations and Techniques.
615 24$aMeasurement Science and Instrumentation.
676   $a523.887
700   $aYuasa$b Takayuki$4aut$4http://id.loc.gov/vocabulary/relators/aut$0871949
906   $aBOOK
912   $a9910437978703321
996   $aSuzaku Studies of White Dwarf Stars and the Galactic X-ray Background Emission$91946819
997   $aUNINA