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- W1991187112 abstract "Joint analysis of Suzaku/Chandra emission/absorption lines were conducted to constrain the density and geometry of hot gas along two lines of sights of LMC X-3 and 4U 1820-303. Because significant foreground line emissions may exist, the Suzaku emission data must be analyzed with spacial cares. The present results imply the hot gas to extend to the galacticdisk scale or more for the LMC X-3 direction. However, the present simple model fails to explain the results for the 4U1820-303 directions." @default.
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- W1991187112 date "2007-01-01" @default.
- W1991187112 modified "2023-09-23" @default.
- W1991187112 title "Suzaku/Chandra Emission/Absorption Line Observations of Hot Gas in and around Our Galaxy" @default.
- W1991187112 doi "https://doi.org/10.1143/ptps.169.79" @default.
- W1991187112 hasPublicationYear "2007" @default.
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