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• W3099789975 endingPage "12" @default.
• W3099789975 startingPage "12" @default.
• W3099789975 abstract "NGC 891 is a nearby edge-on galaxy that is similar to the Milky Way and has a hot X-ray emitting halo that could arise from accretion, a galactic fountain, or a combination of the two. The metallicity of the gas can help distinguish between these models, and here we report on results that use 138 ks of archival Chandra data and 92 ks of new XMM-Newton data to measure the temperature and metallicity of the hot halo of the galaxy. We find good fits for a thermal model with kT ~ 0.2 keV and Z ~ 0.1 solar, and rule out solar metallicity to more than 99% confidence. This result suggests accretion from the intergalactic medium as the origin for the hot halo. However, it is also possible to fit a two-temperature thermal model with solar metallicity where kT_1 = 0.1 keV and kT_2 = 0.25 keV. A consideration of the cooling rate and scale height prefers the single-temperature model. We also find that the cooling rate in the hot gas cannot explain the massive HI halo in the steady state. In addition, a galactic fountain model cannot eject enough mass to account for the HI halo, and we speculate that the neutral halo may be gas from a prior outflow that has since cooled." @default.
• W3099789975 created "2020-11-23" @default.
• W3099789975 creator A5016719102 @default.
• W3099789975 creator A5032147246 @default.
• W3099789975 date "2012-12-07" @default.
• W3099789975 modified "2023-10-18" @default.
• W3099789975 title "A DEEP X-RAY VIEW OF THE HOT HALO IN THE EDGE-ON SPIRAL GALAXY NGC 891" @default.
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• W3099789975 doi "https://doi.org/10.1088/0004-637x/762/1/12" @default.
• W3099789975 hasPublicationYear "2012" @default.
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