任意
发表于 2025-3-23 13:23:47
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Fretful
发表于 2025-3-23 15:53:06
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忧伤
发表于 2025-3-23 18:45:02
2190-5053 ed 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..978-4-431-54717-4978-4-431-54219-3Series ISSN 2190-5053 Series E-ISSN 2190-5061
Morbid
发表于 2025-3-24 00:00:44
Review of the Galactic X-ray Background Emission and White Dwarf Binaries, high sensitivity in the hard X-ray wavelength, which are indispensable for the present study to spectroscopically decompose possible contributions from multiple types of X-ray stars to the GRXE, are described.
Pamphlet
发表于 2025-3-24 04:51:07
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beta-carotene
发表于 2025-3-24 07:13:21
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象形文字
发表于 2025-3-24 12:27:17
Review of the Galactic X-ray Background Emission and White Dwarf Binaries,onting scenarios, the point-source scenario and the truly-diffuse scenario, for the originating source and the emission mechanism of the GRXE are explained. Several recent supports to the point-source origin based on recent X-ray spectroscopic and X-ray high-resolution imaging studies with Chandra a
圆木可阻碍
发表于 2025-3-24 16:52:07
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Legion
发表于 2025-3-24 22:06:48
Instrumentation,d spectral coverage and the high sensitivity on apparently extended emission. Conventional X-ray spectral analysis method adopted in the following chapters is also explained for those who are not familiar with it.
熄灭
发表于 2025-3-25 03:09:49
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