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Suzaku Studies of White Dwarf Stars and the Galactic X-ray Background Emission (eBook)

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2013 | 2013
XV, 154 Seiten
Springer Tokyo (Verlag)
978-4-431-54219-3 (ISBN)

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Suzaku Studies of White Dwarf Stars and the Galactic X-ray Background Emission - Takayuki Yuasa
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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.



Dr. Takayuki Yuasa
Department of Physics, Graduate School of Science
The University of Tokyo, Japan


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.

Dr. Takayuki YuasaDepartment of Physics, Graduate School of ScienceThe University of Tokyo, Japan

Review 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.

Erscheint lt. Verlag 16.1.2013
Reihe/Serie Springer Theses
Springer Theses
Zusatzinfo XV, 154 p.
Verlagsort Tokyo
Sprache englisch
Themenwelt Naturwissenschaften Physik / Astronomie Astronomie / Astrophysik
Technik
Schlagworte Accretion Column • Fe Line from Shock-heated Plasma • Galactic Ridge X-ray Emission (GRXE) • Intermediate Polar • Magnetic White Dwarf Binary • Post Shock Region • Prize winning thesis • White Dwarf Star
ISBN-10 4-431-54219-1 / 4431542191
ISBN-13 978-4-431-54219-3 / 9784431542193
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