| 書目名稱 | Suzaku Studies of White Dwarf Stars and the Galactic X-ray Background Emission |
| 編輯 | Takayuki Yuasa |
| 視頻video | http://file.papertrans.cn/884/883655/883655.mp4 |
| 概述 | Provides an X-ray spectral model that estimates white dwarf masses by fitting observed data from the Suzaku observatory.Reveals that the observed broadband spectra of the Galactic ridge X-ray emission |
| 叢書名稱 | Springer Theses |
| 圖書封面 |  |
| 描述 | .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.. |
| 出版日期 | Book 2013 |
| 關鍵詞 | Accretion Column; Fe Line from Shock-heated Plasma; Galactic Ridge X-ray Emission (GRXE); Intermediate |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-4-431-54219-3 |
| isbn_softcover | 978-4-431-54717-4 |
| isbn_ebook | 978-4-431-54219-3Series ISSN 2190-5053 Series E-ISSN 2190-5061 |
| issn_series | 2190-5053 |
| copyright | Springer Japan 2013 |
|Archiver|手機版|小黑屋|
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