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- W180804988 abstract "We report on the properties of the hot gaseous halos of 10 nearby ultraluminous IRAS galaxies from Chandra observations. There exists diffuse soft X-ray emission surrounding the central nucleus within 10 kpc of the nuclear region with a temperature of about 0.7 keV and metallicity about Z ~ 1.0 Z ⊙ . Also, emission lines from α elements and ions for are seen in all nearby ULIRGs in our sample. Outside the central region, the Chandra observations reveal a more extended hot gaseous halo with a temperature of about 0.6 keV and low metallicity ( Z ~ 0.1 Z ⊙ ) for some of the ULIRGs. We discuss the nature and the implications of our results for the origin of X-ray halos in elliptical galaxies and the constraints this places on the feedback process." @default.
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- W180804988 date "2004-01-01" @default.
- W180804988 modified "2023-09-22" @default.
- W180804988 title "The Galaxy Merger Origin of Hot Gaseous Halos of Ellipticals" @default.
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- W180804988 doi "https://doi.org/10.1017/s0074180900198055" @default.
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